The Astronomy and Astrophysics Review最新文献

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Low-energy cosmic rays: regulators of the dense interstellar medium 低能宇宙射线:密集星际介质的调节器
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-09-03 DOI: 10.1007/s00159-022-00141-2
Stefano Gabici
{"title":"Low-energy cosmic rays: regulators of the dense interstellar medium","authors":"Stefano Gabici","doi":"10.1007/s00159-022-00141-2","DOIUrl":"10.1007/s00159-022-00141-2","url":null,"abstract":"<div><p>Low-energy cosmic rays (up to the GeV energy domain) play a crucial role in the physics and chemistry of the densest phase of the interstellar medium. Unlike interstellar ionising radiation, they can penetrate large column densities of gas, and reach molecular cloud cores. By maintaining there a small but not negligible gas ionisation fraction, they dictate the coupling between the plasma and the magnetic field, which in turn affects the dynamical evolution of clouds and impacts on the process of star and planet formation. The cosmic-ray ionisation of molecular hydrogen in interstellar clouds also drives the rich interstellar chemistry revealed by observations of spectral lines in a broad region of the electromagnetic spectrum, spanning from the submillimetre to the visual band. Some recent developments in various branches of astrophysics provide us with an unprecedented view on low-energy cosmic rays. Accurate measurements and constraints on the intensity of such particles are now available both for the very local interstellar medium and for distant interstellar clouds. The interpretation of these recent data is currently debated, and the emerging picture calls for a reassessment of the scenario invoked to describe the origin and/or the transport of low-energy cosmic rays in the Galaxy.</p></div>","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"30 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-09-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"134795341","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 7
Ram pressure stripping in high-density environments 高密度环境下闸板压力剥离
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-05-18 DOI: 10.1007/s00159-022-00140-3
Alessandro Boselli, Matteo Fossati, Ming Sun
{"title":"Ram pressure stripping in high-density environments","authors":"Alessandro Boselli,&nbsp;Matteo Fossati,&nbsp;Ming Sun","doi":"10.1007/s00159-022-00140-3","DOIUrl":"10.1007/s00159-022-00140-3","url":null,"abstract":"<div><p>Galaxies living in rich environments are suffering different perturbations able to drastically affect their evolution. Among these, ram pressure stripping, i.e. the pressure exerted by the hot and dense intracluster medium (ICM) on galaxies moving at high velocity within the cluster gravitational potential well, is a key process able to remove their interstellar medium (ISM) and quench their activity of star formation. This review is aimed at describing this physical mechanism in different environments, from rich clusters of galaxies to loose and compact groups. We summarise the effects of this perturbing process on the baryonic components of galaxies, from the different gas phases (cold atomic and molecular, ionised, hot) to magnetic fields and cosmic rays, and describe their induced effects on the different stellar populations, with a particular attention to its role in the quenching episode generally observed in high-density environments. We also discuss on the possible fate of the stripped material once removed from the perturbed galaxies and mixed with the ICM, and we try to estimate its contribution to the pollution of the surrounding environment. Finally, combining the results of local and high-redshift observations with the prediction of tuned models and simulations, we try to quantify the importance of this process on the evolution of galaxies of different mass, from dwarfs to giants, in various environments and at different epochs.</p></div>","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"30 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-05-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00159-022-00140-3.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"134796962","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 33
Fast radio bursts at the dawn of the 2020s 本世纪20年代初的快速射电暴
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-03-29 DOI: 10.1007/s00159-022-00139-w
E. Petroff, J. W. T. Hessels, D. R. Lorimer
{"title":"Fast radio bursts at the dawn of the 2020s","authors":"E. Petroff,&nbsp;J. W. T. Hessels,&nbsp;D. R. Lorimer","doi":"10.1007/s00159-022-00139-w","DOIUrl":"10.1007/s00159-022-00139-w","url":null,"abstract":"<div><p>Since the discovery of the first fast radio burst (FRB) in 2007, and their confirmation as an abundant extragalactic population in 2013, the study of these sources has expanded at an incredible rate. In our 2019 review on the subject, we presented a growing, but still mysterious, population of FRBs—60 unique sources, 2 repeating FRBs, and only 1 identified host galaxy. However, in only a few short years, new observations and discoveries have given us a wealth of information about these sources. The total FRB population now stands at over 600 published sources, 24 repeaters, and 19 host galaxies. Higher time resolution data, sustained monitoring, and precision localisations have given us insight into repeaters, host galaxies, burst morphology, source activity, progenitor models, and the use of FRBs as cosmological probes. The recent detection of a bright FRB-like burst from the Galactic magnetar SGR 1935 + 2154 provides an important link between FRBs and magnetars. There also continue to be surprising discoveries, like periodic modulation of activity from repeaters and the localisation of one FRB source to a relatively nearby globular cluster associated with the M81 galaxy. In this review, we summarise the exciting observational results from the past few years. We also highlight their impact on our understanding of the FRB population and proposed progenitor models. We build on the introduction to FRBs in our earlier review, update our readers on recent results, and discuss interesting avenues for exploration as the field enters a new regime where hundreds to thousands of new FRBs will be discovered and reported each year.</p></div>","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"30 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-03-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00159-022-00139-w.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"5127726","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 69
The growing threat of light pollution to ground-based observatories 光污染对地面天文台的威胁日益严重
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-01-27 DOI: 10.1007/s00159-021-00138-3
Richard F. Green, Christian B. Luginbuhl, Richard J. Wainscoat, Dan Duriscoe
{"title":"The growing threat of light pollution to ground-based observatories","authors":"Richard F. Green,&nbsp;Christian B. Luginbuhl,&nbsp;Richard J. Wainscoat,&nbsp;Dan Duriscoe","doi":"10.1007/s00159-021-00138-3","DOIUrl":"10.1007/s00159-021-00138-3","url":null,"abstract":"<div><p>Human activity is rapidly increasing the negative impact of artificial skyglow at even the most remote professional observatory sites. Assessment of the actual impact requires an understanding of the propagation as a function of source spectral energy distribution. The higher blue content of light-emitting diodes being widely used as replacement for sodium discharge lamps has greater impact closer to the source, and less impact for more distant mountain-top sites. All-sky cameras with moderate angular resolution provide data and metrics sufficient to model and remove celestial contributions and provide measures of artificial light contribution. The natural skyglow is significantly affected by solar activity, which must be accounted for in determining secular trends in the artificial component. With the availability of the New World Atlas of the Artificial Sky Brightness, a direct comparison is made of the modeled artificial contribution to the sites with the largest aperture telescopes, noting the possible systematic errors in individual cases. Population growth of the nearest urban centers allows a prediction of the change in that brightness over a decade. All site protections are effected primarily by national or regional regulation. A collection of worldwide regulations shows that most are leveraged off environmental protection statutes, while in the U.S., they are largely based on land-use zones. Particular examples are presented in more detail for Flagstaff, Arizona, and the Island of Hawai’i. The latest rapidly growing threat is that of reflected sunlight from large constellations of satellites in low-earth orbit. A snapshot is provided of that rapidly changing situation. In all cases, astronomers must become very proactive in educating the public about the cultural value of visual or naked eye astronomy as well as the science and the need for access to a dark night sky for astronomical research.</p></div>","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"30 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-01-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00159-021-00138-3.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"5042255","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 23
A Brief Review on the Research of Testing of Cosmological Principle 宇宙原理检验研究述评
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-01-01 DOI: 10.12677/aas.2022.104004
宇航 唐
{"title":"A Brief Review on the Research of Testing of Cosmological Principle","authors":"宇航 唐","doi":"10.12677/aas.2022.104004","DOIUrl":"https://doi.org/10.12677/aas.2022.104004","url":null,"abstract":"This paper presents a brief introduction on the research of testing of cosmological principles","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"2013 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"86206853","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
How Gravity Is Produced?—Lines of Gravitation Are Deflecting the Direction of Motion of an Object 重力是如何产生的?引力线使物体的运动方向发生偏转
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-01-01 DOI: 10.12677/aas.2022.102002
军利 陈
{"title":"How Gravity Is Produced?—Lines of Gravitation Are Deflecting the Direction of Motion of an Object","authors":"军利 陈","doi":"10.12677/aas.2022.102002","DOIUrl":"https://doi.org/10.12677/aas.2022.102002","url":null,"abstract":"","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"60 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"84550201","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 1
Gravity, Gravitational Fields, and Gravitons—Inference about the Frequency of Gravitational Energy Waves 重力、引力场和引力子——关于引力波频率的推断
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-01-01 DOI: 10.12677/aas.2022.101001
军利 陈
{"title":"Gravity, Gravitational Fields, and Gravitons—Inference about the Frequency of Gravitational Energy Waves","authors":"军利 陈","doi":"10.12677/aas.2022.101001","DOIUrl":"https://doi.org/10.12677/aas.2022.101001","url":null,"abstract":"Through the analysis of resonance, this paper puts forward an inference about gravitation: gravitation is an energy wave with a frequency of 1.875 × 10^23 Hz, its frequency is higher than that of gamma rays, and it can penetrate any matter. The smallest unit of gravitation is proton and neutral Sub (nucleon), each proton and neutron (nucleon) unit (1 s) time can emit a maximum of 0.937 × 10^23 graviton, the diameter of the graviton is less than 10^−20 m, the gravitational force","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"47 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"82594966","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 1
The Hubble Constant Tension in Cosmology 宇宙学中的哈勃恒张力
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2022-01-01 DOI: 10.12677/aas.2022.103003
术银 杨
{"title":"The Hubble Constant Tension in Cosmology","authors":"术银 杨","doi":"10.12677/aas.2022.103003","DOIUrl":"https://doi.org/10.12677/aas.2022.103003","url":null,"abstract":"This paper briefly introduces the tension of Hubble constant measurements and its related progresses. Firstly, we show several normal methods of the measurement of Hubble constant. Se-condly, we present the results of the Hubble constant measurement in the recent twenty years,","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"16 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2022-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"87865774","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
A buyer’s guide to the Hubble constant 哈勃常数的买家指南
IF 27.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2021-12-01 DOI: 10.1007/s00159-021-00137-4
Paul Shah, Pablo Lemos, Ofer Lahav
{"title":"A buyer’s guide to the Hubble constant","authors":"Paul Shah,&nbsp;Pablo Lemos,&nbsp;Ofer Lahav","doi":"10.1007/s00159-021-00137-4","DOIUrl":"10.1007/s00159-021-00137-4","url":null,"abstract":"<div><p>Since the expansion of the universe was first established by Edwin Hubble and Georges Lemaître about a century ago, the Hubble constant <span>(H_0)</span> which measures its rate has been of great interest to astronomers. Besides being interesting in its own right, few properties of the universe can be deduced without it. In the last decade, a significant gap has emerged between different methods of measuring it, some anchored in the nearby universe, others at cosmological distances. The SH0ES team has found <span>(H_0 = 73.2 pm 1.3 ; ;,hbox {kms}^{-1} ,hbox {Mpc}^{-1})</span> locally, whereas the value found for the early universe by the Planck Collaboration is <span>(H_0 = 67.4 pm 0.5 ; ;,hbox {kms}^{-1} ,hbox {Mpc}^{-1})</span> from measurements of the cosmic microwave background. Is this gap a sign that the well-established <span>({varLambda} {text{CDM}})</span> cosmological model is somehow incomplete? Or are there unknown systematics? And more practically, how should humble astronomers pick between competing claims if they need to assume a value for a certain purpose? In this article, we review results and what changes to the cosmological model could be needed to accommodate them all. For astronomers in a hurry, we provide a buyer’s guide to the results, and make recommendations.</p></div>","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"29 1","pages":""},"PeriodicalIF":27.8,"publicationDate":"2021-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s00159-021-00137-4.pdf","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138514251","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Rotation of an oblate satellite: Chaos control (Corrigendum) 一个扁圆卫星的旋转:混沌控制(勘误)
IF 25.8 1区 物理与天体物理
The Astronomy and Astrophysics Review Pub Date : 2021-11-01 DOI: 10.1051/0004-6361/201731167E
M. Tarnopolski
{"title":"Rotation of an oblate satellite: Chaos control (Corrigendum)","authors":"M. Tarnopolski","doi":"10.1051/0004-6361/201731167E","DOIUrl":"https://doi.org/10.1051/0004-6361/201731167E","url":null,"abstract":"","PeriodicalId":785,"journal":{"name":"The Astronomy and Astrophysics Review","volume":"21 1","pages":""},"PeriodicalIF":25.8,"publicationDate":"2021-11-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"90593524","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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