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相关论文: Hot Evolved Stars in the Centers of M 31 and M 32

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We present Faint Object Camera (FOC) ultraviolet images of the central 14x14'' of Messier 31 and Messier 32. The hot stellar population detected in the composite UV spectra of these nearby galaxies is partially resolved into individual…

天体物理学 · 物理学 2009-10-30 T. M. Brown , H. C. Ferguson , S. A. Stanford , J. -M. Deharveng

The compact elliptical galaxy M32 offers a unique testing ground for theories of stellar evolution. Because of its proximity, solar-blind UV observations can resolve the hot evolved stars in its center. Some of these late evolutionary…

天体物理学 · 物理学 2007-05-23 Thomas M. Brown , Henry C. Ferguson , Allen V. Sweigart , Randy A. Kimble , Charles W. Bowers

Using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope, we have obtained deep far-ultraviolet images of the compact elliptical galaxy M32. When combined with earlier near-ultraviolet images of the same field, these…

We present the deepest near-UV image of M32 to date, which for the first time resolves hot HB stars in an elliptical galaxy. Given the near-solar metallicity of M32, much larger than that of globular clusters, the existence of an extended…

天体物理学 · 物理学 2009-10-31 Thomas M. Brown , Charles W. Bowers , Randy A. Kimble , Allen V. Sweigart , Henry C. Ferguson

As part of the Panchromatic Hubble Andromeda Treasury (PHAT) multi-cycle program, we observed a 12' \times 6.5' area of the bulge of M31 with the WFC3/UVIS filters F275W and F336W. From these data we have assembled a sample of \sim4000…

We present the result of a survey for star clusters in M33 using the HST/WFPC2 archive images. We have found 104 star clusters, including 32 new ones, in the images of 24 fields that were not included in the previous studies. Combining…

天体物理学 · 物理学 2008-11-26 Won-Kee Park , Myung Gyoon Lee

Using the Canada-France-Hawaii Telescope we have obtained deep high-resolution CCD images in V and I of a 28'x28' field in the outer disk of M 31 at ~ 116' from the center along the major axis to the south-west, and covering a range of…

天体物理学 · 物理学 2009-11-06 Jean-Charles Cuillandre , James Lequeux , Ronald J. Allen , Yannick Mellier , Emmanuel Bertin

We present a catalog of 2,990 extended sources in a 1deg x1deg area centered on M33 using the MegaCam camera on the 3.6m Canada-France-Hawaii telescope (CFHT). The catalog includes 599 new candidate stellar clusters, 204 previously…

星系天体物理 · 物理学 2015-05-19 Izaskun San Roman , Ata Sarajedini , Antonio Aparicio

We present deep color-magnitude diagrams (CMDs) for a field along the outer disk of M31 based on archival Hubble Space Telescope Wide Field Planetary Camera 2 observations in the F555W (~V) and F814W (~I) filters. The CMDs, which contain a…

天体物理学 · 物理学 2007-05-23 Ata Sarajedini , Jeffrey Van Duyne

We have carried out a search for above-horizontal-branch (AHB) stars--objects lying above the horizontal branch (HB) and blueward of the asymptotic giant branch (AGB) in the color-magnitude diagram--in 97 Galactic and seven Magellanic Cloud…

太阳与恒星天体物理 · 物理学 2022-02-23 Brian D. Davis , Howard E. Bond , Michael H. Siegel , Robin Ciardullo

We have imaged five 7\arcmin \x 7\arcmin\ fields in M31 spanning galactocentric radii from 4 to 32 kpc along the SW-major axis. The fields were observed through two broad-band (\V\ and \I) and two narrow-band (\CN\ and \TiO) filters. The…

天体物理学 · 物理学 2016-08-30 J. P. Brewer , H. B. Richer , D. R. Crabtree

Variable stars in stellar clusters can offer key constraints on stellar evolution and pulsation models, utilising estimates of host cluster properties to constrain stellar physical parameters. We present a catalogue of 86 luminous…

We have performed a census of the UV-bright population in 78 globular clusters using wide-field UV telescopes. This population includes a variety of phases of post-horizontal branch (HB) evolution, including hot post-asymptotic giant branch…

太阳与恒星天体物理 · 物理学 2019-07-03 S. Moehler , W. B. Landsman , T. Lanz , M. M. Miller Bertolami

We have conducted a near-infrared monitoring campaign at the UK InfraRed Telescope, of the Local Group spiral galaxy M33. The main aim was to identify stars in the very final stage of their evolution, and for which the luminosity is more…

星系天体物理 · 物理学 2016-10-04 Atefeh Javadi , Jacco van Loon , Habib Khosroshahi

We present a far-ultraviolet (FUV) study of hot stellar populations in the second parameter pair globular clusters (GCs) M3 and M13, as a part of the Globular cluster UVIT Legacy Survey program (GlobULeS). We use observations made with…

太阳与恒星天体物理 · 物理学 2023-04-10 Ranjan Kumar , Ananta C. Pradhan , Snehalata Sahu , Annapurni Subramaniam , Sonika Piridi , Santi Cassisi , Devendra K. Ojha

This study presents an investigation of nearly two dozen candidate Luminous Blue Variables (cLBVs) in the galaxies M31 and M33. Eight stars have been studied in detail, while an additional sixteen objects are briefly mentioned. Multi-epoch…

太阳与恒星天体物理 · 物理学 2026-03-12 Sai Li , Cheng Liu , Jincheng Guo

We present a CCD investigation of the galactic globular M5 aimed to increase the statistical relevance of the available sample of evolving bright stars. Previous investigations, limited to the outer cluster region, have been extended toward…

天体物理学 · 物理学 2009-10-22 E. Brocato , V. Castellani , V. Ripepi

We present photometry for all bright red giant branch (RGB), horizontal branch (HB), and asymptotic giant branch (AGB) stars within 10' of the center of M13. We find support for the idea that the population of HB stars redder than the…

太阳与恒星天体物理 · 物理学 2015-05-18 Eric L. Sandquist , Mark Gordon , Daniel Levine , Michael Bolte

We present the first detection of 24 {\mu}m variability in 24 sources in the Local Group galaxy M33. These results are based on 4 epochs of MIPS observations, which are irregularly spaced over ~750 days. We find that these sources are…

太阳与恒星天体物理 · 物理学 2015-06-23 Edward J. Montiel , Sundar Srinivasan , Geoffrey C. Clayton , Charles W. Engelbracht , Christopher B. Johnson

We present the first results of a survey of blue horizontal branch (BHB) stars in the Galactic bulge. 164 candidates with 15 < V < 17.5 in a field 7.5deg from the Galactic Center were observed in the blue at 2.4A FWHM resolution with the…

天体物理学 · 物理学 2009-10-31 Ruth C. Peterson , Donald M. Terndrup , Elaine M. Sadler , Alistair R. Walker
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