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Status: Bibliographieeintrag

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Verfasst von:Larson, Kirsten [VerfasserIn]   i
 Lee, Janice C [VerfasserIn]   i
 Thilker, David A [VerfasserIn]   i
 Whitmore, Bradley C [VerfasserIn]   i
 Deger, Sinan [VerfasserIn]   i
 Lilly, James [VerfasserIn]   i
 Chandar, Rupali [VerfasserIn]   i
 Dale, Daniel A [VerfasserIn]   i
 Bigiel, Frank [VerfasserIn]   i
 Grasha, Kathryn [VerfasserIn]   i
 Groves, Brent [VerfasserIn]   i
 Hannon, Stephen [VerfasserIn]   i
 Klessen, Ralf S. [VerfasserIn]   i
 Kreckel, Kathryn [VerfasserIn]   i
 Kruijssen, J M Diederik [VerfasserIn]   i
 Leroy, Adam K [VerfasserIn]   i
 Pan, Hsi-An [VerfasserIn]   i
 Rosolowsky, Erik [VerfasserIn]   i
 Schinnerer, Eva [VerfasserIn]   i
 Schruba, Andreas [VerfasserIn]   i
 Watkins, Elizabeth J. [VerfasserIn]   i
 Williams, Thomas G [VerfasserIn]   i
Titel:Multiscale stellar associations across the star formation hierarchy in PHANGS-HST nearby galaxies
Titelzusatz:methodology and properties
Verf.angabe:Kirsten L Larson, Janice C Lee, David A Thilker, Bradley C Whitmore, Sinan Deger, James Lilly, Rupali Chandar, Daniel A Dale, Frank Bigiel, Kathryn Grasha, Brent Groves, Stephen Hannon, Ralf S Klessen, Kathryn Kreckel, J M Diederik Kruijssen, Adam K Leroy, Hsi-An Pan, Erik Rosolowsky, Eva Schinnerer, Andreas Schruba, Elizabeth J Watkins, Thomas G Williams
E-Jahr:2023
Jahr:August 2023
Umfang:21 S.
Illustrationen:Illustrationen
Fussnoten:Veröffentlicht: 06. Juni 2023 ; Gesehen am 11.10.2023
Titel Quelle:Enthalten in: Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society
Ort Quelle:Oxford : Oxford Univ. Press, 1827
Jahr Quelle:2023
Band/Heft Quelle:523(2023), 4 vom: Aug., Seite 6061-6081
ISSN Quelle:1365-2966
Abstract:We develop a method to identify and determine the physical properties of stellar associations using Hubble Space Telescope (HST) NUV−U−B−V−I imaging of nearby galaxies from the Physics at High Angular Resolution in Nearby GalaxieS with the Hubble Space Telescope (PHANGS-HST) survey. We apply a watershed algorithm to density maps constructed from point source catalogues Gaussian smoothed to multiple physical scales from 8 to 64 pc. We develop our method on two galaxies that span the distance range in the PHANGS-HST sample: NGC 3351 (10 Mpc) and NGC 1566 (18 Mpc). We test our algorithm with different parameters such as the choice of detection band for the point source catalogue (NUV or V), source density image filtering methods, and absolute magnitude limits. We characterize the properties of the resulting multiscale associations, including sizes, number of tracer stars, number of associations, and photometry, as well as ages, masses, and reddening from spectral energy distribution fitting. Our method successfully identifies structures that occupy loci in the UBVI colour-colour diagram consistent with previously published catalogues of clusters and associations. The median ages of the associations increase from log(age/yr) = 6.6 to log(age/yr) = 6.9 as the spatial scale increases from 8 to 64 pc for both galaxies. We find that the youngest stellar associations, with ages <3 Myr, indeed closely trace H ii regions in H α imaging, and that older associations are increasingly anticorrelated with the H α emission. Owing to our new method, the PHANGS-HST multiscale associations provide a far more complete census of recent star formation activity than found with previous cluster and compact association catalogues.
DOI:doi:10.1093/mnras/stad1600
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext: https://doi.org/10.1093/mnras/stad1600
 Volltext: https://academic.oup.com/mnras/article/523/4/6061/7191271
 DOI: https://doi.org/10.1093/mnras/stad1600
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1861524269
Verknüpfungen:→ Zeitschrift

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