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相关论文: Resolving Stellar Populations outside the Local Gr…

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We present deep BVRI CCD photometry of the stars in the dwarf irregular galaxy UKS 2323-326 in the Sculptor Group. The color-magnitude diagrams of the measured stars in UKS 2323-326 show a blue plume which consists mostly of young stellar…

天体物理学 · 物理学 2009-10-31 Myung Gyoon Lee , Yong-Ik Byun

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

太阳与恒星天体物理 · 物理学 2015-05-27 Atefeh Javadi , Jacco Th. van Loon , Mohammad Taghi Mirtorabi

We have traced the spatial distributions of intermediate-age and old stars in nine dwarf galaxies in the distant parts of the Local Group, using multi-epoch 3.6 and 4.5 micron data from the DUST in Nearby Galaxies with Spitzer (DUSTiNGS)…

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 present deep $BVI$ observations of the dwarf irregular galaxy UKS1927-177 in Sagittarius. Statistically cleaned $V$, $(B-I)$ CMDs clearly display the key evolutionary features in this galaxy. Previously detected C stars are located in…

天体物理学 · 物理学 2009-11-07 Y. Momany , E. V. Held , I. Saviane , L. Rizzi

Deep g'r'i'z' images obtained with the Gemini Multi-Object Spectrograph are used to investigate the stellar content in the outer regions of the nearby Sc galaxies NGC 2403 and M33. The red giant branch tip occurs at i' = 23.6 +/- 0.1 in NGC…

天体物理学 · 物理学 2009-11-07 T. J. Davidge

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

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 V and I photometry of the resolved stars in the cometary dwarf irregular galaxy NGC 2366, using Wide Field Planetary Camera 2 images obtained with the Hubble Space Telescope. The resulting color-magnitude diagram reaches down to…

天体物理学 · 物理学 2009-11-10 T. X. Thuan , Y. I. Izotov

In this paper, we show that the optically bright stars above the tip of the first red giant branch (TRGB) in the color magnitude (CM) diagrams of nearby dwarf elliptical (dE) galaxies, commonly interpreted as indication of the existence of…

天体物理学 · 物理学 2009-10-30 D. Martinez-Delgado , A. Aparicio

We present a moderately-deep JK photometry for three selected areas of the dwarf irregular galaxy IC1613. The color-magnitude diagrams contain a mixture of red supergiants, asymptotic giant branch stars and the brightest red giant stars.…

天体物理学 · 物理学 2007-05-23 J. Borissova , L. Georgiev , R. Kurtev , M. Rosado , V. D. Ivanov , M. Richer , M. Valdez-Gutierrez

We present resolved-star VI photometry of the Local Group dwarf irregular galaxy IC1613 reaching I~23.5, obtained with the wide-field camera at the 2.5m Isaac Newton Telescope. A fit to the stellar density distribution shows an exponential…

We have extended the study of the young star clusters observed in the merger remnant galaxy NGC 7252 by obtaining K band photometry for these clusters. Our K band data significantly complement the optical photometry and spectroscopy in the…

天体物理学 · 物理学 2009-11-06 C. Maraston , M. Kissler-Patig , J. P. Brodie , P. Barmby , J. P. Huchra

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

太阳与恒星天体物理 · 物理学 2015-05-19 Atefeh Javadi , Jacco Th. van Loon , Mohammad Taghi Mirtorabi

A near-infrared imaging study of the evolved stellar populations in the dwarf spheroidal galaxy Leo I is presented. Based on JHK observations obtained with the WFCAM wide-field array at the UKIRT telescope, we build a near-infrared…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. V. Held , M. Gullieuszik , L. Rizzi , L. Girardi , P. Marigo , I. Saviane

Near-infrared images obtained with the CFHT AOB are used to investigate the stellar content of the Local Group elliptical galaxy M32. Observations of a field 2.3 arcmin from the galaxy center reveal a large population of AGB stars, and…

天体物理学 · 物理学 2009-10-31 T. J. Davidge

Wide-field JHKs near-infrared observations covering an area of 1.8x1.8 sq. deg. centred on M33 were obtained using WFCAM at UKIRT. These data show a large population of intermediate-age asymptotic giant branch stars (AGB). We have used both…

天体物理学 · 物理学 2009-11-13 M. -R. L. Cioni , M. Irwin , A. M. N. Ferguson , A. McConnachie , B. C. Conn , A. Huxor , R. Ibata , G. Lewis , N. Tanvir

In this contribution initial results from colour-magnitude diagrams for five dEs in the M81 group are presented. The colour-magnitude diagrams, derived from HST/ACS images, reach well below the red giant branch tip and allow evaluation of…

天体物理学 · 物理学 2007-05-23 G. S. Da Costa

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

太阳与恒星天体物理 · 物理学 2015-06-23 Atefeh Javadi , Maryam Saberi , Jacco Th. van Loon , Habib Khosroshahi , Najmeh Golabatooni , Mohammad Taghi Mirtorabi

Asymptotic giant branch stars are essential contributors to the near and mid-IR emission of intermediate age (0.1-1Gyr old) stellar populations. Detecting this light sets constraints on the star formation history in galaxies and,…

天体物理学 · 物理学 2007-05-23 A. Lancon
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