Search Results - "Neugent, Kathryn F."
-
1
A Modern Search for Wolf-Rayet Stars in the Magellanic Clouds. IV. A Final Census
Published in The Astrophysical journal (20-08-2018)“…Abstract We summarize the results of our 4 yr survey searching for Wolf-Rayet (WR) stars in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud. Over…”
Get full text
Journal Article -
2
The Time-averaged Mass-loss Rates of Red Supergiants as Revealed by Their Luminosity Functions in M31 and M33
Published in The Astrophysical journal (01-01-2023)“…Abstract Mass loss in red supergiants (RSGs) is generally recognized to be episodic, but mass-loss prescriptions fail to reflect this. Evolutionary models show…”
Get full text
Journal Article -
3
Newly Discovered Wolf–Rayet Stars in M31
Published in The Astronomical journal (01-08-2023)“…Abstract The evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that…”
Get full text
Journal Article -
4
A Survey for C ii Emission-line Stars in the Large Magellanic Cloud. II. Final Results and the Origin of C ii Emission in [WC] Spectra
Published in The Astrophysical journal (01-01-2023)“…Abstract We present the final results of an imaging and spectroscopic search for stars in the Large Magellanic Cloud (LMC) with C ii λλ 7231, 7236 emission…”
Get full text
Journal Article -
5
Constraints on the Binarity of the WN3/O3 Class of Wolf–Rayet Stars
Published in The Astrophysical journal (01-04-2023)“…Abstract The WN3/O3 Wolf–Rayet (WR) stars were discovered as part of our survey for WRs in the Magellanic Clouds. The WN3/O3s show the emission lines of a…”
Get full text
Journal Article -
6
Physical Properties of 5000 Cool Large Magellanic Cloud Supergiants with Gaia XP Spectra: A Detailed Portrait of the Upper H-R Diagram Hints at Missing Supernova Progenitors
Published in The Astrophysical journal (01-12-2023)“…Abstract Characterizing the physical properties of cool supergiants allows us to probe the final stages of a massive star’s evolution before it undergoes core…”
Get full text
Journal Article -
7
The Luminosity Function of Red Supergiants in M31
Published in The Astrophysical journal (20-01-2020)“…The mass-loss rates of red supergiant stars (RSGs) are poorly constrained by direct measurements, and yet the subsequent evolution of these stars depends…”
Get full text
Journal Article -
8
Binary Yellow Supergiants in the Magellanic Clouds. I. Photometric Candidate Identification
Published in The Astrophysical journal (01-11-2024)“…Abstract Recent works have constrained the binary fraction of evolved populations of massive stars in local galaxies such as red supergiants and Wolf–Rayet…”
Get full text
Journal Article -
9
Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II. Spectroscopic and Environmental Analysis of Thorne–Żytkow Object and Super-AGB Star Candidates
Published in The Astrophysical journal (01-01-2023)“…Abstract In previous work, we identified a population of 38 cool and luminous variable stars in the Magellanic Clouds and examined 11 in detail in order to…”
Get full text
Journal Article -
10
Yellow Supergiants in the Small Magellanic Cloud: Putting Current Evolutionary Theory to the Test
Published in The Astrophysical journal (20-08-2010)“…The yellow supergiant content of nearby galaxies provides a critical test of massive star evolutionary theory. While these stars are the brightest in a galaxy,…”
Get full text
Journal Article -
11
The Red Supergiant Binary Fraction as a Function of Metallicity in M31 and M33
Published in The Astrophysical journal (01-02-2021)“…Recent work measuring the binary fraction of evolved red supergiants (RSGs) in the Magellanic Clouds points to a value between 15% and 30%, with the majority…”
Get full text
Journal Article -
12
A MODERN SEARCH FOR WOLF–RAYET STARS IN THE MAGELLANIC CLOUDS. II. A SECOND YEAR OF DISCOVERIES
Published in The Astrophysical journal (01-07-2015)“…The numbers and types of evolved massive stars found in nearby galaxies provide an exacting test of stellar evolution models. Because of their proximity and…”
Get full text
Journal Article -
13
THE CLOSE BINARY FREQUENCY OF WOLF-RAYET STARS AS A FUNCTION OF METALLICITY IN M31 AND M33
Published in The Astrophysical journal (01-07-2014)“…Massive star evolutionary models generally predict the correct ratio of WC-type and WN-type Wolf-Rayet stars at low metallicities, but underestimate the ratio…”
Get full text
Journal Article -
14
A MODERN SEARCH FOR WOLF-RAYET STARS IN THE MAGELLANIC CLOUDS: FIRST RESULTS
Published in The Astrophysical journal (10-06-2014)“…Over the years, directed surveys and incidental spectroscopy have identified 12 Wolf-Rayet (WR) stars in the Small Magellanic Cloud (SMC) and 139 in the Large…”
Get full text
Journal Article -
15
A Modern Search for Wolf-Rayet Stars in the Magellanic Clouds. III. A Third Year of Discoveries
Published in The Astrophysical journal (10-03-2017)“…For the past three years we have been conducting a survey for Wolf-Rayet (WR) stars in the Large and Small Magellanic Clouds (LMC, SMC). Our previous work…”
Get full text
Journal Article -
16
The Wolf-Rayet Content of M33
Published in The Astrophysical journal (01-06-2011)“…Wolf-Rayet (WR) stars are evolved massive stars, and the relative number of WC-type and WN-type WRs should vary with metallicity, providing a sensitive test of…”
Get full text
Journal Article -
17
YELLOW AND RED SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD
Published in The Astrophysical journal (20-04-2012)“…Due to their transitionary nature, yellow supergiants (YSGs) provide a critical challenge for evolutionary modeling. Previous studies within M31 and the Small…”
Get full text
Journal Article -
18
The Red Supergiant Binary Fraction of the Large Magellanic Cloud
Published in The Astrophysical journal (01-09-2020)“…The binary fraction of unevolved massive stars is thought to be 70%-100% but there are few observational constraints on the binary fraction of the evolved…”
Get full text
Journal Article -
19
The Evolution and Physical Parameters of WN3/O3s: A New Type of Wolf–Rayet Star
Published in The Astrophysical journal (20-05-2017)“…Abstract As part of a search for Wolf–Rayet (WR) stars in the Magellanic Clouds, we have discovered a new type of WR star in the Large Magellanic Cloud (LMC)…”
Get full text
Journal Article -
20
Binary Red Supergiants. II. Discovering and Characterizing B-type Companions
Published in The Astrophysical journal (20-04-2019)“…The percentage of massive main-sequence OB stars in binary systems is thought to be as high as 100%. However, very few Galactic binary red supergiants (RSGs)…”
Get full text
Journal Article