Journal
ASTRONOMICAL JOURNAL
Volume 145, Issue 6, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/145/6/149
Keywords
galaxies: distances and redshifts; galaxies: dwarf; galaxies: irregular; galaxies: photometry; galaxies: stellar content
Categories
Funding
- NSF Faculty Early Career Development (CAREER) award [AST-0847109]
- NSF [AST-0607007, AST-1107390, AST-1211683]
- Brinson Foundation
- National Aeronautics and Space Administration
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1211683] Funding Source: National Science Foundation
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1107390, 0847109] Funding Source: National Science Foundation
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We present results from ground-based optical imaging of a low-mass dwarf galaxy discovered by the ALFALFA 21 cm Hi survey. Broadband (BVR) data obtained with the WIYN 3.5 m telescope at Kitt Peak National Observatory (KPNO) are used to construct color-magnitude diagrams of the galaxy's stellar population down to V-o similar to 25. We also use narrowband H alpha imaging from the KPNO 2.1 m telescope to identify a H II region in the galaxy. We use these data to constrain the distance to the galaxy to be between 1.5 and 2.0 Mpc. This places Leo P within the Local Volume but beyond the Local Group. Its properties are extreme: it is the lowest-mass system known that contains significant amounts of gas and is currently forming stars.
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