The Astrophysical Journal Letters最新文献

{"title":"Orthogonal Alignment of Galaxy Group Angular Momentum with Cosmic Filament Spines: An Observational Study","authors":"Yu Rong, Peng Wang and Xiao-xiao Tang","doi":"10.3847/2041-8213/adc130","DOIUrl":"https://doi.org/10.3847/2041-8213/adc130","url":null,"abstract":"We investigated the alignment between the angular momenta of galaxy groups and the spines of their associated cosmic filaments. Our results demonstrate a significant tendency for these two orientations to be perpendicular, indicating that the rotation of a galaxy group does not originate from the spin of cosmic filaments. Instead, it is driven by the orbital angular momentum contributed by member galaxies as they accrete along the direction of the filament spines. Moreover, the strength of this perpendicular alignment signal varies with the richness of the galaxy groups, with the most pronounced alignment observed among the wealthiest groups. This pronounced alignment is largely due to the more coherent spatial distribution of member galaxies in richer groups relative to the filament spines. Our study provides valuable insights into the mechanisms of angular momentum acquisition in galaxy groups from an observational standpoint.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"58 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143766445","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Improving Photometric Redshifts of Epoch of Reionization Galaxies: A New Empirical Transmission Curve with Neutral Hydrogen Damping Wing Lyα Absorption","authors":"Yoshihisa Asada, Guillaume Desprez, Chris J. Willott, Marcin Sawicki, Maruša Bradač, Gabriel Brammer, Florian Dubath, Kartheik G. Iyer, Nicholas S. Martis, Adam Muzzin, Gaël Noirot, Stéphane Paltani, Ghassan T. E. Sarrouh, Anishya Harshan and Vladan Markov","doi":"10.3847/2041-8213/adc388","DOIUrl":"https://doi.org/10.3847/2041-8213/adc388","url":null,"abstract":"We present a new analytical model for the attenuation to Epoch of Reionization (EoR) galaxies by proximate neutral hydrogen gas. Many galaxy spectra in the EoR taken by JWST have shown a flux deficit at wavelengths just redward of the Lyman break, and this has been regarded as resulting from Lyα damping wing absorption by the increasing amount of neutral hydrogen in the line of sight. However, previous attenuation models for the intergalactic medium (IGM) commonly used in photometric redshift template-fitting codes assume that the Lyman break is rather sharp, which leads to systematic overestimation of photometric redshifts at z > 7. In this Letter, we build and empirically calibrate a new attenuation model that takes the increased Lyα damping wing absorption into account. Our model consists of the canonical IGM absorption and an additional absorption component due to dense neutral hydrogen gas clouds proximate to the galaxy, and we derive the redshift evolution of H i column density of the proximate clouds by calibrating the model using CANUCS JWST observations. The resulting total transmission curve resolves the photometric redshift bias at z > 7, an improvement that is robust to the choice of template-fitting code, template set, and photometric catalog used. The new attenuation model can be easily implemented in existing template-fitting codes and significantly improves the photometric redshift performance in the EoR.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"62 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143766446","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Exotic Nanophase Iron as a New Agent for Space Weathering on the Moon","authors":"Xiaojia Zeng, Xiaoping Zhang, Yanxue Wu, Wen Yu, Xiongyao Li and Jianzhong Liu","doi":"10.3847/2041-8213/adbf88","DOIUrl":"https://doi.org/10.3847/2041-8213/adbf88","url":null,"abstract":"Nanophase iron (np-Fe) particles in space-weathered lunar regolith are widely concerning as they can change the spectral, chemical, and physical properties of lunar soils. These np-Fe particles were previously believed to be produced from lunar surface materials by space weathering processes, while the source of np-Fe particles from exotic micrometeorite (flux = ∼5 × 108 t/Ma) has been overlooked. In this study, we report the discovery of np-Fe particles in the micrometeorite impactor residue on a plagioclase crystal from Chang’e-5 lunar soil. Our results show that the source of these np-Fe particles does not originate from lunar materials, but rather are sourced from micrometeorites (i.e., exotic origin). This work provides mineralogical evidence that exotic np-Fe particles can be delivered and preserved by micrometeorite impact melting and reduction on the Moon. The estimated production rate of exotic np-Fe particles is as high as ∼5 × 106 t/Ma on the Moon. We therefore suggest that these exotic np-Fe particles have a nonnegligible influence on the interpretation of the space weathering process in special environments (e.g., permanently shadowed regions) of the Moon and other airless planetary bodies in the solar system.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"183 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143775682","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Space Weathering Properties of Chang’e-6 Soils and Implication for Regolith Evolution of Young Lunar Maria","authors":"Xuejin Lu, Jian Chen, Haijun Cao, Changqing Liu, Ziyi Jia, Chengxiang Yin, Tianwei Wang, Xiaohui Fu, Le Qiao, Xiaojia Zeng, Jiang Zhang and Zongcheng Ling","doi":"10.3847/2041-8213/adbffc","DOIUrl":"https://doi.org/10.3847/2041-8213/adbffc","url":null,"abstract":"Lunar soil samples from young maria (formed <3.0 billion years ago (Ga)) preserve key records of recent space weathering history in the Earth–Moon system. China’s Chang’e-6 mission returned the first farside soil samples from a young mare (∼2.8 Ga) at the northeastern South Pole–Aitken basin. We present preliminary results on the space weathering properties of the Chang’e-6 soils. The glassy agglutinate content in the Chang’e-6 soils is approximately 30%, significantly lower than the 50%–70% observed in the mature Apollo soils from older maria (>3.0 Ga) and higher than the ∼21% found in the Chang’e-5 soils from younger mare (∼2.0 Ga). However, our spectroscopic study reveals that the Chang’e-6 soils are well developed, with high maturity, weak absorption, and a red-sloped continuum, similar to the characteristics of the mature soils from the Apollo and Chang’e-5 landing sites. Orbital observations indicate more mature surface than in the returned samples from young mare regions, likely due to the destruction of an optically mature veneer by spacecraft. The optically mature veneer reveals deficiencies in remote sensing and emphasizes the importance of sample return missions. The thinner optically mature veneer and lower abundance of glassy agglutinate in younger maria suggest reduced gardening cycles and changes in impactor properties (such as rate and size) after 3.0 Ga. This is important for understanding how the relative contributions of space weathering agents change over time and the evolution of impactors in the inner solar system.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"23 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143766444","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Cosmic Evolution Early Release Science Survey (CEERS)","authors":"Steven L. Finkelstein, Micaela B. Bagley, Pablo Arrabal Haro, Mark Dickinson, Henry C. Ferguson, Jeyhan S. Kartaltepe, Dale D. Kocevski, Anton M. Koekemoer, Jennifer M. Lotz, Casey Papovich, Pablo G. Pérez-González, Nor Pirzkal, Rachel S. Somerville, Jonathan R. Trump, Guang Yang, L. Y. Aaron Yung, Adriano Fontana, Andrea Grazian, Norman A. Grogin, Lisa J. Kewley, Allison Kirkpatrick, Rebecca L. Larson, Laura Pentericci, Swara Ravindranath, Stephen M. Wilkins, Omar Almaini, Ricardo O. Amorín, Guillermo Barro, Rachana Bhatawdekar, Laura Bisigello, Madisyn Brooks, Véronique Buat, Fernando Buitrago, Denis Burgarella, Antonello Calabrò, Marco Castellano, Yingjie Cheng, Nikko J. Cleri, Justin W. Cole, M. C. Cooper, Olivia R. Cooper, Luca Costantin, Isa G. Cox, Darren Croton, Emanuele Daddi, Kelcey Davis, Avishai Dekel, David Elbaz, Vital Fernández, Seiji Fujimoto, Giovanni Gandolfi, Jonathan P. Gardner, Eric Gawiser, Mauro Giavalisco, Carlos Gómez-Guijarro, Yuchen Guo, Ansh R. Gup..","doi":"10.3847/2041-8213/adbbd3","DOIUrl":"https://doi.org/10.3847/2041-8213/adbbd3","url":null,"abstract":"We present the Cosmic Evolution Early Release Science (CEERS) Survey, a 77.2 hr Director’s Discretionary Early Release Science Program. CEERS demonstrates, tests, and validates efficient extragalactic surveys using coordinated, overlapping parallel observations with the JWST instrument suite, including NIRCam and MIRI imaging, NIRSpec low- (R ∼ 100) and medium- (R ∼ 1000) resolution spectroscopy, and NIRCam slitless grism (R ∼ 1500) spectroscopy. CEERS targets the Hubble Space Telescope–observed region of the Extended Groth Strip field, supported by a rich set of multiwavelength data. CEERS facilitated immediate community science in both of the extragalactic core JWST science drivers “First Light” and “Galaxy Assembly,” including: (1) the discovery and characterization of large samples of galaxies at z ≳ 10 from ∼90 arcmin2 of NIRCam imaging, constraining their abundance and physical nature; (2) deep spectra of >1000 galaxies, including dozens of galaxies at 6 < z < 10, enabling redshift measurements and constraints on the physical conditions of star formation and black hole growth via line diagnostics; (3) quantifying the first bulge, bar, and disk structures at z > 3; and (4) characterizing galaxy mid-IR emission with MIRI to study dust-obscured star formation and supermassive black hole growth at z ∼ 1–3. As a legacy product for the community, the CEERS team has provided several data releases, accompanied by detailed notes on the data reduction procedures and notebooks to aid in reproducibility. In addition to an overview of the survey and the quality of the data, we provide science highlights from the first two years with CEERS data.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"216 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-04-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143775702","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"On the Anisotropic Velocity Distribution of Newborn Pickup Ions in the Heliosheath","authors":"Senbei Du, Merav Opher and Marc Kornbleuth","doi":"10.3847/2041-8213/adbc9a","DOIUrl":"https://doi.org/10.3847/2041-8213/adbc9a","url":null,"abstract":"The evolution of the velocity distribution of pickup ions is crucial for understanding the energetic neutral atom (ENA) fluxes observed by Interstellar Boundary Explorer. Pickup ions in the heliosheath contain two main components: those transmitted across the heliospheric termination shock and those locally created within the heliosheath. In this work, we discuss the velocity distribution of the latter locally created component. We find that pickup ions created by the charge exchange of neutral solar wind (NSW) may be a significant source of the observed ENA fluxes between about 100 eV and 1 keV. Moreover, newborn pickup ions can maintain highly anisotropic velocity distribution in the heliosheath. This is because the kinetic instabilities are weak after the solar wind flow decelerates at the termination shock. Hybrid kinetic simulations show the mirror instability to be the dominant mode for conditions in the heliosheath close to the termination shock. We estimate that effects of NSW and anisotropy may enhance the expected phase space density of newborn pickup ions by more than a factor of 100.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"107 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143758692","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Lyman Continuum Leakers at z > 3 in the GOODS-S Field: Mergers Dominated","authors":"Shuairu Zhu, 帅儒 朱, Zhen-Ya Zheng, Fang-Ting Yuan, Chunyan Jiang and Ruqiu Lin","doi":"10.3847/2041-8213/adc125","DOIUrl":"https://doi.org/10.3847/2041-8213/adc125","url":null,"abstract":"Understanding the ionizing photon escape from galaxies is essential for studying cosmic reionization. With a sample of 23 Lyman continuum (LyC) leakers (among which eight are high-confidence leakers) at 3 < z < 4.5 in the GOODS-S field, we investigate their morphologies using high-resolution data from the Hubble Space Telescope and the James Webb Space Telescope. We find that 20 of the 23 LyC leakers (seven out of eight high-confidence leakers) show merging signatures via visual inspection, while the remaining three are starbursts. The merger fraction of our sample is significantly higher than that of normal galaxies at similar or higher redshifts. Even when using the nonparametric method, which may miss some mergers in a sample, the merger fraction remains high, especially for the high-confidence leakers. Based on our previous finding that LyC leakers are not necessarily starbursts while some are in the star formation main sequence, we further find that those in the main sequence show merger signatures. Our results suggest that LyC leakers are either starbursts or mergers, both of which can facilitate the LyC photon escape, in addition to generating more LyC photons. Furthermore, we show that high-z LyC leakers are statistically more extended than those selected at low redshift, which exhibit a higher merger fraction as size increases. This is likely due to the observational bias that the spatial resolution limits the detection of high-z compact galaxies, while low redshift LyC leakers are more selected as compact starbursts.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"73 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-03-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143758359","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"A Rotational Disruption Crisis for Zodiacal Dust","authors":"Kedron Silsbee, Brandon S. Hensley, Jamey R. Szalay, Petr Pokorný and Jeong-Gyu Kim","doi":"10.3847/2041-8213/adc133","DOIUrl":"https://doi.org/10.3847/2041-8213/adc133","url":null,"abstract":"A systematic torque from anisotropic radiation can rapidly spin up irregular grains to the point of breakup. We apply the standard theory of rotational disruption from radiative torques to solar system grains, finding that grains with radii ∼0.03–3 μm at 1 au from the Sun are spun to the point of breakup on timescales ≲1 yr even when assuming them to have an unrealistically high tensile strength of pure meteoritic iron. Such a rapid disruption timescale is incompatible with both the abundance of micron-sized grains detected in the inner solar system and with the low production rate of β-meteoroids. We suggest the possibility that zodiacal grains have a strong propensity to attain rotational equilibrium at low angular velocity (a so-called low-J attractor) and that the efficacy of rotational disruption in the solar system—and likely elsewhere—has been greatly overestimated.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"72 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-03-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736824","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Red Supergiant Progenitor of the Type II Supernova 2024abfl","authors":"Jingxiao Luo, Lifu Zhang, Bing-Qiu Chen, Qiyuan Cheng, Boyang Guo, Jiao Li, Yanjun Guo, Jianping Xiong, Xiangcun Meng, Xuefei Chen, Zhengwei Liu and Zhanwen Han","doi":"10.3847/2041-8213/adbf0b","DOIUrl":"https://doi.org/10.3847/2041-8213/adbf0b","url":null,"abstract":"Linkage between core-collapse supernovae and their progenitors is not fully understood and ongoing effort of searching and identifying the progenitors is needed. SN 2024abfl is a recent Type II supernova that exploded in the nearby star-bursting galaxy NGC 2146, which is also the host galaxy of SN 2018zd. From archival Hubble Space Telescope data, we have found a red source (mF814W ∼ 25) near the location (angular distance ≤0 2) of SN 2024abfl before its explosion. With F814W and F606W photometry, we found that the properties of this source matched a typical red supergiant (RSG) moderately reddened by interstellar dust at the distance of the host galaxy. We conclude that the SN 2024abfl had an RSG progenitor with initial mass of 9 –12 M⊙.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"36 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-03-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736826","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Black Hole Pulsars and Monster Shocks as Outcomes of Black Hole–Neutron Star Mergers","authors":"Yoonsoo Kim, Elias R. Most, Andrei M. Beloborodov and Bart Ripperda","doi":"10.3847/2041-8213/adbff9","DOIUrl":"https://doi.org/10.3847/2041-8213/adbff9","url":null,"abstract":"The merger of a black hole (BH) and a neutron star (NS) in most cases is expected to leave no material around the remnant BH; therefore, such events are often considered as sources of gravitational waves without electromagnetic counterparts. However, a bright counterpart can emerge if the NS is strongly magnetized, as its external magnetosphere can experience radiative shocks and magnetic reconnection during/after the merger. We use magnetohydrodynamic simulations in the dynamical spacetime of a merging BH–NS binary to investigate its magnetospheric dynamics. We find that compressive waves excited in the magnetosphere develop into monster shocks as they propagate outward. After swallowing the NS, the BH acquires a magnetosphere that quickly evolves into a split-monopole configuration and then undergoes an exponential decay (balding), enabled by magnetic reconnection and also assisted by the ringdown of the remnant BH. This spinning BH drags the split monopole into rotation, forming a transient pulsar-like state. It emits a striped wind if the swallowed magnetic-dipole moment is inclined to the spin axis. We predict two types of transients from this scenario: (1) a fast radio burst emitted by the shocks as they expand to large radii; and (2) an X-ray/γ-ray burst emitted by the e± outflow heated by magnetic dissipation.","PeriodicalId":501814,"journal":{"name":"The Astrophysical Journal Letters","volume":"102 4 Pt 1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2025-03-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143736823","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}