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相关论文: Anomalous Stellar Populations in LSB Galaxies

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We present WFC3 observations of three low surface brightness (LSB) galaxies from the Schombert et. al LSB catalog that are within 11 Mpc of the Milky Way. Deep imaging at F336W, F555W and F814W allow the construction of the V-I…

星系天体物理 · 物理学 2015-08-19 J. Schombert , S. McGaugh

We present near-infrared (NIR) color-magnitude diagrams (CMDs) for the resolved stellar populations within 26 fields of 23 nearby galaxies (<4 Mpc), based on F110W and F160W images from Wide Field Camera 3 (WFC3) on the Hubble Space…

We report the discovery of four extremely faint ($m_{\mathrm{F444W}}\gtrsim29$) red point sources in recent ultra-deep JWST/NIRCam images of the strong lensing galaxy cluster Abell S1063. All four sources sit in lensed arcs, on the symmetry…

We have observed the closest known large, low surface brightness (LSB) galaxy, UGC 2302, with HST using WFPC2 and the F555W and F814W filters. UGC 2302 is a typical large LSB galaxy, and thus represents a good choice for detailed stellar…

天体物理学 · 物理学 2007-05-23 Patricia M. Knezek

Multiple stellar populations (MPs) are a distinct characteristic of Globular Clusters (GCs). Their general properties have been widely studied among main sequence, red giant branch (RGB) and horizontal branch (HB) stars, but a common…

太阳与恒星天体物理 · 物理学 2021-03-31 E. P. Lagioia , A. P. Milone , A. F. Marino , M. Tailo , A. Renzini , M. Carlos , G. Cordoni , E. Dondoglio , S. Jang , A. Karakas , A. Dotter

Spectroscopy and V,I CCD photometry of the dwarf irregular galaxy SBS 1129+576 are presented for the first time. The CCD images reveal a chain of compact H II regions within the elongated low-surface-brightness (LSB) component of the…

天体物理学 · 物理学 2009-11-07 N. G. Guseva , P. Papaderos , Y. I. Izotov , R. F. Green , K. J. Fricke , T. X. Thuan , K. J. Noeske

We investigate the star formation history of the central regions of four Luminous Compact Blue Galaxies (LCBGs). LCBGs are blue (B-V<0.6), compact (MU_B<21.5 mag arcsec^-2) galaxies with absolute magnitudes M_B brighter than -17.5. The…

天体物理学 · 物理学 2008-11-26 C. Hoyos , R. Guzman , A. I. Diaz , D. C. Koo , M. A. Bershady , .

We present the third and final part of a census of Asymptotic Giant Branch (AGB) stars in Local Group dwarf irregular galaxies. Papers I and II presented the results for WLM and IC 1613. Included here are Phoenix, LGS 3, DDO 210, Leo A,…

星系天体物理 · 物理学 2011-02-11 Martha L. Boyer , Evan D. Skillman , Jacco Th. van Loon , Robert D. Gehrz , Charles E. Woodward

A series of population models are designed to explore the star formation history of gas-rich, low surface brightness (LSB) galaxies. LSB galaxies are unique in having properties of very blue colors, low H$\alpha$ emission and high gas…

星系天体物理 · 物理学 2015-06-22 James Schombert , Stacy McGaugh

In the I-band color-magnitude diagrams (CMD) of resolved nearby galaxies, the reddest asymptotic giant branch (AGB) stars form a previously unremarked-upon, but nevertheless distinct and easily-identified population of high-luminosity…

太阳与恒星天体物理 · 物理学 2026-02-17 Barry F. Madore , Wendy L. Freedman , Taylor Hoyt , In Sung Jang , Abigail Lee , Kayla Owens

Galactic Globular clusters (GCs) are now known to harbour multiple stellar populations, which are chemically distinct in many light element abundances. It is becoming increasingly clear that asymptotic giant branch (AGB) stars in GCs show…

太阳与恒星天体物理 · 物理学 2016-04-27 B. T. MacLean , S. W. Campbell , G. M. De Silva , J. Lattanzio , V. DOrazi , J. D. Simpson , Y. Momany

Galactic globular clusters (GCs) are known to host multiple stellar populations: a first generation with a chemical pattern typical of halo field stars and a second generation (SG) enriched in Na and Al and depleted in O and Mg. Both…

太阳与恒星天体物理 · 物理学 2015-12-09 D. A. Garcia-Hernandez , Sz. Meszaros , M. Monelli , S. Cassisi , P. B. Stetson , O. Zamora , M. Shetrone , S. Lucatello

This paper presents optical and H-alpha imaging for a large sample of LSB galaxies selected from the PSS-II catalogs (Schombert et. al 1992). As noted in previous work, LSB galaxies span a range of luminosities (-10 > M_V > -20) and sizes…

宇宙学与河外天体物理 · 物理学 2014-05-28 James Schombert , Tamela Maciel , Stacy McGaugh

Aims. This study focuses on very luminous Mbol<-6.0 mag AGB stars with J-Ks>1.5 mag and H-Ks>0.4 mag in the LMC, SMC, M31, and M33 from 2MASS data. Methods.The data were taken from the 2MASS All-Sky Point Source catalogue archive. We used…

天体物理学 · 物理学 2016-08-30 P. Tsalmantza , E. Kontizas , L. Cambresy , F. Genova , A. Dapergolas , M. Kontizas

The huge photometric databases that are being created for stars in the Magellanic Clouds and in Local Group galaxies not only allow detailed study of the star formation history of these systems, but also provide important information on…

天体物理学 · 物理学 2009-10-30 Carme Gallart

We calculated theoretical evolutionary sequences of asymptotic giant branch (AGB) stars, including formation and evolution of dust grains in their circumstellar envelope. By considering stellar populations of the Large Magellanic Cloud…

太阳与恒星天体物理 · 物理学 2016-08-10 F. Dell'Agli , P. Ventura , R. Schneider , M. Di Criscienzo , D. A. García-Hernández , C. Rossi , E. Brocato

We present Spitzer/IRAC observations at 3.6 and 4.5 microns along with optical data from the Local Group Galaxies Survey to investigate the evolved stellar population of the Local Group dwarf irregular galaxy WLM. These observations provide…

天体物理学 · 物理学 2008-11-26 Dale C. Jackson , Evan D. Skillman , Robert D. Gehrz , Elisha Polomski , Charles E. Woodward

We investigate the utility of the asymptotic giant branch (AGB) and the red giant branch (RGB) as probes of the star formation history (SFH) of the nearby (D=2.5 Mpc) dwarf irregular galaxy, KKH 98. Near-infrared (IR) Keck Laser Guide Star…

宇宙学与河外天体物理 · 物理学 2015-05-18 J. Melbourne , B. Williams , J. Dalcanton , S. M. Ammons , C. Max , D. C. Koo , Leo Girardi , A. Dolphin

We investigate the population of cool, evolved stars in the Local Group dwarf elliptical galaxy M32, using Infrared Array Camera observations from the Spitzer Space Telescope. We construct deep mid-infrared colour-magnitude diagrams for the…

太阳与恒星天体物理 · 物理学 2015-06-23 O. C. Jones , I. McDonald , R. M. Rich , F. Kemper , M. L. Boyer , A. A. Zijlstra , G. J. Bendo

Outskirts of large galaxies contain important information about the galaxy formation and assembly process, and resolved star count studies can probe the extremely low surface brightness of the outer halos. We use images obtained with the…

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