Newly Discovered Wolf–Rayet Stars in M31

The evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that the Wolf–Rayet (WR) content of M31 may have been underestimated. We therefore began a pilot project to search for new WRs in M31 and to reexamine the...

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Main Authors: Kathryn F. Neugent, Philip Massey
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/ace25f
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author Kathryn F. Neugent
Philip Massey
author_facet Kathryn F. Neugent
Philip Massey
author_sort Kathryn F. Neugent
collection DOAJ
description The evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that the Wolf–Rayet (WR) content of M31 may have been underestimated. We therefore began a pilot project to search for new WRs in M31 and to reexamine the completeness of our previous WR survey, finished almost a decade prior. Our improved imaging data and spectroscopic follow-up confirmed 19 new WRs across three small fields in M31. These newly discovered WRs are generally fainter than the previously known sample due to slightly increased reddening as opposed to intrinsic faintness. From these findings, we estimate that there are another ∼60 WRs left to be discovered in M31; however, the overall ratio of WN-type (nitrogen-rich) to WC-type (carbon-rich) WRs remains unchanged with our latest additions to the M31 WR census. We are in the process of extending this pilot WR survey to include the rest of M31, and a more complete population will be detailed in our future work.
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spelling doaj.art-0f3de9058c1a4a06b1b7bf8636fd72062023-09-03T15:07:13ZengIOP PublishingThe Astronomical Journal1538-38812023-01-0116626810.3847/1538-3881/ace25fNewly Discovered Wolf–Rayet Stars in M31Kathryn F. Neugent0https://orcid.org/0000-0002-5787-138XPhilip Massey1https://orcid.org/0000-0001-6563-7828Center for Astrophysics, Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138, USA ; Kathryn.Neugent@cfa.harvard.eduLowell Observatory , 1400 W Mars Hill Road, Flagstaff, AZ 86001, USA; Department of Astronomy and Planetary Science, Northern Arizona University , Flagstaff, AZ 86011-6010, USAThe evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that the Wolf–Rayet (WR) content of M31 may have been underestimated. We therefore began a pilot project to search for new WRs in M31 and to reexamine the completeness of our previous WR survey, finished almost a decade prior. Our improved imaging data and spectroscopic follow-up confirmed 19 new WRs across three small fields in M31. These newly discovered WRs are generally fainter than the previously known sample due to slightly increased reddening as opposed to intrinsic faintness. From these findings, we estimate that there are another ∼60 WRs left to be discovered in M31; however, the overall ratio of WN-type (nitrogen-rich) to WC-type (carbon-rich) WRs remains unchanged with our latest additions to the M31 WR census. We are in the process of extending this pilot WR survey to include the rest of M31, and a more complete population will be detailed in our future work.https://doi.org/10.3847/1538-3881/ace25fWolf-Rayet starsMassive starsEvolved starsAndromeda GalaxyStellar populations
spellingShingle Kathryn F. Neugent
Philip Massey
Newly Discovered Wolf–Rayet Stars in M31
The Astronomical Journal
Wolf-Rayet stars
Massive stars
Evolved stars
Andromeda Galaxy
Stellar populations
title Newly Discovered Wolf–Rayet Stars in M31
title_full Newly Discovered Wolf–Rayet Stars in M31
title_fullStr Newly Discovered Wolf–Rayet Stars in M31
title_full_unstemmed Newly Discovered Wolf–Rayet Stars in M31
title_short Newly Discovered Wolf–Rayet Stars in M31
title_sort newly discovered wolf rayet stars in m31
topic Wolf-Rayet stars
Massive stars
Evolved stars
Andromeda Galaxy
Stellar populations
url https://doi.org/10.3847/1538-3881/ace25f
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