L. R. Bedin, D. Nardiello, M. Salaris, M. Libralato, P. Bergeron, A. J. Burgasser, D. Apai, M. Griggio, M. Scalco, J. Anderson, R. Gerasimov, A. Bellini
{"title":"JWST imaging of the closest globular clusters—I. Possible infrared excess among white dwarfs in NGC 6397","authors":"L. R. Bedin, D. Nardiello, M. Salaris, M. Libralato, P. Bergeron, A. J. Burgasser, D. Apai, M. Griggio, M. Scalco, J. Anderson, R. Gerasimov, A. Bellini","doi":"10.1002/asna.20240039","DOIUrl":null,"url":null,"abstract":"<p>We present <i>James Webb Space Telescope</i> observations of the globular cluster NGC 6397 and use them to extend to infrared wavelengths the characterization of the cluster's entire white dwarf (WD) cooling sequence (CS). The data allows us to probe fundamental astrophysical WD properties and to search for evidence in their colors for (or against) the existence of ancient planetary systems. The existing archival <i>Hubble Space Telescope</i> imaging data obtained <span></span><math>\n <semantics>\n <mrow>\n <mo>∼</mo>\n <mn>18</mn>\n </mrow>\n <annotation>$$ \\sim 18 $$</annotation>\n </semantics></math> years ago reach ultra-deep optical magnitudes (<span></span><math>\n <semantics>\n <mrow>\n <mi>V</mi>\n <mo>∼</mo>\n <mn>31</mn>\n </mrow>\n <annotation>$$ V\\sim 31 $$</annotation>\n </semantics></math>) and allow us to derive a near-perfect separation between field and cluster members. We detect an apparent split in the lower part of the WD CS of NGC 6397. The red part of the WD CS, containing about 25% of the total, exhibits significant IR-excess of up to <span></span><math>\n <semantics>\n <mrow>\n <mi>Δ</mi>\n <msub>\n <mi>m</mi>\n <mrow>\n <mi>F</mi>\n <mn>322</mn>\n <mi>W</mi>\n <mn>2</mn>\n </mrow>\n </msub>\n <mo>∼</mo>\n <mn>0.5</mn>\n </mrow>\n <annotation>$$ \\Delta {m}_{\\mathrm{F}322\\mathrm{W}2}\\sim 0.5 $$</annotation>\n </semantics></math> mag. These infrared excesses require both theoretical and observational follow-ups to confirm their veracity and to ascertain their true nature.</p>","PeriodicalId":55442,"journal":{"name":"Astronomische Nachrichten","volume":"345 6-7","pages":""},"PeriodicalIF":1.1000,"publicationDate":"2024-05-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomische Nachrichten","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/asna.20240039","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
We present James Webb Space Telescope observations of the globular cluster NGC 6397 and use them to extend to infrared wavelengths the characterization of the cluster's entire white dwarf (WD) cooling sequence (CS). The data allows us to probe fundamental astrophysical WD properties and to search for evidence in their colors for (or against) the existence of ancient planetary systems. The existing archival Hubble Space Telescope imaging data obtained years ago reach ultra-deep optical magnitudes () and allow us to derive a near-perfect separation between field and cluster members. We detect an apparent split in the lower part of the WD CS of NGC 6397. The red part of the WD CS, containing about 25% of the total, exhibits significant IR-excess of up to mag. These infrared excesses require both theoretical and observational follow-ups to confirm their veracity and to ascertain their true nature.
期刊介绍:
Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.