An Extensive Catalog of Early-type Dwarf Galaxies in the Local Universe: Morphology and Environment

被引:10
|
作者
Paudel, Sanjaya [1 ]
Yoon, Suk-Jin [1 ]
Yoo, Jaewon [2 ]
Smith, Rory [2 ]
Chhatkuli, Daya Nidhi [3 ]
Bachchan, Rajesh Kumar [4 ]
Aryal, Binil [3 ]
Adhikari, Binod [4 ,5 ]
Adhikari, Namuna [3 ]
Sedain, Amrit [3 ]
Sheikh, Sharup [3 ]
Dhital, Sarashwati [3 ]
Giri, Ashutosh [5 ]
Baral, Rabin [5 ]
机构
[1] Yonsei Univ, Dept Astron, Seoul 03722, South Korea
[2] Korea Astron & Space Sci Inst KASI, 776 Daedeokdae ro, Daejeon 34055, South Korea
[3] Tribhuvan Univ, Cent Dept Phys, Kirtipur, Kathmandu, Nepal
[4] Tribhuvan Univ, Patan Multiple Coll, Dept Phys, Kathmandu, Nepal
[5] Tribhuvan Univ, St Xaviers Coll, Dept Phys, Kathmandu, Nepal
来源
基金
新加坡国家研究基金会; 美国国家科学基金会; 美国国家航空航天局;
关键词
ULTRA-DIFFUSE GALAXIES; GENERATION VIRGO CLUSTER; DIGITAL SKY SURVEY; ABSOLUTE MAGNITUDE RELATION; NUCLEAR STAR-CLUSTERS; LOW-MASS GALAXIES; ELLIPTIC GALAXIES; TIDAL INTERACTION; EVOLUTION; ORIGIN;
D O I
10.3847/1538-4365/acbfa7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an extensive catalog of 5405 early-type dwarf (dE) galaxies located in the various environments, i.e., clusters, groups, and fields, of the local universe (z < 0.01). The dEs are selected through visual inspection of the Legacy survey's g-r-z combined tricolor images. The inspected area, covering a total sky area of 7643 deg(2), encompasses two local clusters (Virgo and Fornax), 265 groups, and the regions around 586 field galaxies of M-K < -21 mag. The catalog aims to be one of the most extensive and publicly accessible collections of data on dEs, despite its complex completeness limits, which may not accurately represent its statistical completeness. The strength of the catalog lies in the morphological characteristics, including nucleated, tidal, and ultradiffuse dEs. The two clusters contribute nearly half (2437 out of 5405) of the dEs, and the 265 groups contribute 2103 dEs. There are 864 dEs in 586 fields, i.e., similar to 1.47 dEs per field. Using a standard definition commonly used in literature, we identify 100 ultradiffuse galaxies (UDGs), which compose similar to 2% of the dE population. We find that 40% of our sample dEs harbor a central nucleus, and among the UDG population, a majority (79%) are nonnucleated. About 1.3% of dEs suffer from ongoing tidal disturbance by nearby massive galaxies, and only 0.03% show a sign of recent dwarf-dwarf mergers. The association between dEs and their nearest bright neighbor galaxies suggests that dEs are more likely created where their neighbors are non-star-forming ones.
引用
收藏
页数:14
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