Distances to 24 Dwarf Galaxies

IF 1.3 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
N. A. Tikhonov, O. A. Galazutdinova
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引用次数: 0

Abstract

Absrtact

Stellar photometry of 24 dwarf galaxies was carried out using the archival images of the Hubble Space Telescope. The resulting Hertzsprung–Russell diagrams reveal branches of young and old stars. Using the results of photometry and applying the TRGB method, we have for the first time determined exact distances to 13 galaxies. Galaxy PGC 704814 is located at the closest distance (\(D = 3.73\) Mpc), while SDSS J115 840.37+153 533.7 is located the farthest from us (\(D = 11.95\) Mpc). The distances to other galaxies lie in the range from 7 to 11 Mpc. The object SDSS J140 457.78+534 128.2, as follows from the distribution of red giants, is not a galaxy, but rather a young star complex on the periphery of the neighboring galaxy NGC 5474.

Abstract Image

24个矮星系的距离
摘要利用哈勃太空望远镜的档案图像,对24个矮星系进行了恒星光度测量。由此产生的赫茨普龙-罗素图揭示了年轻恒星和年老恒星的分支。利用光度测量的结果和TRGB方法,我们首次确定了13个星系的精确距离。星系PGC 704814离我们最近(\(D = 3.73\) Mpc),而SDSS J115 840.37+153 533.7离我们最远(\(D = 11.95\) Mpc)。它与其他星系的距离在7到11百万光年之间。根据红巨星的分布,SDSS J140 457.78+534 128.2不是一个星系,而是邻近星系NGC 5474外围的一个年轻的恒星复合体。
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来源期刊
Astrophysical Bulletin
Astrophysical Bulletin 地学天文-天文与天体物理
CiteScore
2.00
自引率
33.30%
发文量
31
审稿时长
>12 weeks
期刊介绍: Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.
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