FIRST RESULTS FROM THE MADCASH SURVEY: A FAINT DWARF GALAXY COMPANION TO THE LOW-MASS SPIRAL GALAXY NGC 2403 AT 3.2 MPC

被引:81
作者
Carlin, Jeffrey L. [1 ,2 ,3 ]
Sand, David J. [4 ]
Price, Paul [5 ]
Willman, Beth [1 ,2 ,3 ]
Karunakaran, Ananthan [6 ]
Spekkens, Kristine [6 ,7 ]
Bell, Eric F. [8 ]
Brodie, Jean P. [9 ]
Crnojevic, Denija [4 ]
Forbes, Duncan A. [10 ]
Hargis, Jonathan [11 ]
Kirby, Evan [12 ]
Lupton, Robert [5 ]
Peter, Annika H. G. [13 ,14 ]
Romanowsky, Aaron J. [9 ,15 ]
Strader, Jay [16 ]
机构
[1] LSST, 933 North Cherry Ave, Tucson, AZ 85721 USA
[2] Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA
[3] Haverford Coll, Dept Astron, 370 Lancaster Ave, Haverford, PA 19041 USA
[4] Texas Tech Univ, Dept Phys, Box 41051, Lubbock, TX 79409 USA
[5] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[6] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON K7L 3N6, Canada
[7] Royal Mil Coll Canada, Dept Phys, POB 17000, Kingston, ON K7L 7B4, Canada
[8] Univ Michigan, Dept Astron, 1085 South Univ Ave, Ann Arbor, MI 48109 USA
[9] Univ Calif Observ, 1156 High St, Santa Cruz, CA 95064 USA
[10] Swinburne Univ, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[11] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[12] CALTECH, 1200 E Calif Blvd,MC 249-17, Pasadena, CA 91125 USA
[13] Ohio State Univ, Dept Phys, CCAPP, 174 W 18th Ave, Columbus, OH 43210 USA
[14] Ohio State Univ, Dept Astron, 174 W 18Th Ave, Columbus, OH 43210 USA
[15] San Jose State Univ, Dept Phys & Astron, One Washington Sq, San Jose, CA 95192 USA
[16] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
dark matter; galaxies: dwarf; galaxies: formation; galaxies: halos; MILKY-WAY SATELLITES; STAR-FORMATION RATES; DIGITAL SKY SURVEY; RED GIANT BRANCH; LOCAL VOLUME; LAMBDA-CDM; HALO; DISCOVERY; DARK; SIMULATIONS;
D O I
10.3847/2041-8205/828/1/L5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of the faintest known dwarf galaxy satellite of a Large Magellanic Cloud (LMC) stellar-mass host beyond the Local Group (LG), based on deep imaging with Subaru/Hyper Suprime-Cam. Magellanic Analog Dwarf Companions And Stellar Halos (MADCASH). J074238+652501-dw lies similar to 35 kpc in projection from NGC 2403, a dwarf spiral galaxy at D approximate to 3.2 Mpc. This new dwarf has Mg = -7.4 +/- 0.4 and a half- light radius of 168 +/- 70. pc, at the calculated distance of 3.39 +/- 0.41 Mpc. The color-magnitude diagram reveals no evidence of young stellar populations, suggesting that MADCASH. J074238+652501-dw is an old, metal-poor dwarf similar to low-luminosity dwarfs in the LG. The lack of either detected HI gas (M-HI/L-V < 0.69M circle dot/L circle dot,based on Green Bank Telescope observations) or GALEX NUV/FUV flux enhancement is consistent with a lack of young stars. This is the first result from the MADCASH survey, which is conducting a census of the stellar substructure and faint satellites in the halos of Local Volume LMC analogs via resolved stellar populations. Models predict a total of similar to 4-10 satellites at least as massive as MADCASH. J074238+652501-dw around a host with the mass of NGC 2403, with 2-3 within our field of view, slightly more than the one such satellite observed in our footprint.
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