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相关论文: The AGB population in IC 1613 using JHK photometry

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We are going to apply AGB stars to find star formation history for IC\,1613 galaxy, this a new and simple method that works well for nearby galaxies. IC\,1613 is a Local Group dwarf irregular galaxy that is located at distance of 750 kpc, a…

星系天体物理 · 物理学 2017-12-19 Seyed Azim Hashemi , Atefeh Javadi , Jacco Th. van Loon

We present Spitzer Space Telescope IRAC photometry of the Local Group dwarf irregular galaxy IC 1613. We compare our 3.6, 4.5, 5.8, and 8.0 micron photometry with broadband optical photometry and find that the optical data do not detect 43%…

天体物理学 · 物理学 2009-11-13 Dale C. Jackson , Evan D. Skillman , Robert D. Gehrz , Elisha Polomski , Charles E. Woodward

NGC 6822 is an irregular dwarf galaxy and part of the Local Group. Its close proximity and apparent isolation provide a unique opportunity to study galactic evolution without any obvious strong external influences. This paper aims to study…

宇宙学与河外天体物理 · 物理学 2015-06-04 L. F. Sibbons , S. G. Ryan , M. -R. L. Cioni M. Irwin , R. Napiwotzki

The metallicity gradient and the stellar distribution within the Local Group dwarf galaxy NGC 6822 has been studied photometrically using asymptotic branch stars (AGB). In order to study the stellar and metallicity distribution, the carbon-…

太阳与恒星天体物理 · 物理学 2010-11-22 L. F. Sibbons , M. -R. L. Cioni , M. Irwin , M. Rejkuba

We used models of thermally-pulsing asymptotic giant branch (AGB) stars, that also describe the dust-formation process in the wind, to interpret the combination of near- and mid-infrared photometric data of the dwarf galaxy IC 1613. This is…

太阳与恒星天体物理 · 物理学 2016-06-08 F. Dell'Agli , M. Di Criscienzo , M. L. Boyer , D. A. Garcia-Hernandez

IC 1613 is a Local Group dwarf irregular galaxy at a distance of 750 kpc. In this work, we present an analysis of the star formation history (SFH) of a field of $\sim200$ square arcmin in the central part of the galaxy. To this aim, we use…

星系天体物理 · 物理学 2018-12-19 Seyed Azim Hashemi , Atefeh Javadi , Jacco Th. van Loon

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

We have observed the center of the Local Group dwarf irregular galaxy IC 1613 with WFPC2 aboard the Hubble Space Telescope in the F439W, F555W, and F814W filters. We find a dominant old stellar population (aged ~7 Gyr), identifiable by the…

JHKs photometry is presented from a three-year survey of the central regions of the Local Group dwarf irregular galaxy IC1613. The morphologies of the colour-magnitude and colour-colour diagrams are discussed with particular reference to…

星系天体物理 · 物理学 2015-08-06 John W. Menzies , Patricia A. Whitelock , Michael W. Feast

We investigate the star formation history and metallicity of the Local Group irregular dwarf galaxy WLM using wide-field JHK near-infrared imaging, spanning a region of approximately 1 sq. degree, obtained with WFCAM on UKIRT. JHK…

太阳与恒星天体物理 · 物理学 2010-11-12 Benjamin Tatton , Maria-Rosa Cioni , Mike Irwin

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 present the spectral analysis of 21 blue supergiant stars of spectral type late B to early A within the Local Group dwarf galaxy IC 1613 based on VLT-FORS2 low resolution spectra. Combining our results with studies of early B type blue…

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

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 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

We study the Galactic distribution of ~10,000 Asymptotic Giant Branch (AGB) stars selected by IRAS colors and variability index. The distance to each star is estimated by assuming a narrow luminosity function and a model-derived bolometric…

天体物理学 · 物理学 2009-11-07 T. Jackson , Z. Ivezic , G. R. Knapp

IC 1613 is an isolated dwarf galaxy within the Local Group. Low foreground and internal extinction, low metallicity, and low crowding make it an invaluable testbed for the calibration of the local distance ladder. We present new,…

We report a spectroscopic study on red supergiant stars (RSGs) in the irregular dwarf galaxy IC 1613 in the Local Group. We derive the effective temperatures ($T_\mathrm{eff}$) and metallicities of 14 RSGs by synthetic spectral fitting to…

星系天体物理 · 物理学 2022-11-09 Sang-Hyun Chun , Sung-Chul Yoon , Heeyoung Oh , Byeong-Gon Park , Narae Hwang

J, H, and K' images are used to investigate the asymptotic giant branch (AGB) content of the Local Group dwarf elliptical galaxy NGC 205. The AGB on the (K, H-K) and (K, J-K) color-magnitude diagrams consists of two sequences: a…

天体物理学 · 物理学 2009-11-10 T. J. Davidge

Hubble Space Telescope (HST) observations of 92 galaxies that have a strong showing of I-band Asymptotic Giant Branch (IAGB) stars in their color-magnitude diagrams (CMDs), are used to measure the relative offset between the mean apparent…

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