Published December 2015
| Published
Journal Article
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Limits on the H I content of the dwarf galaxy Hydra II
Abstract
Sensitive 21 cm H I observations have been made with the Green Bank Telescope toward the newly-discovered Local Group dwarf galaxy Hydra II, which may lie within the leading arm of the Magellanic Stream. No neutral hydrogen was detected. Our 5σ limit of M_(HI) ≤ 210 M_⊙ for a 15 km s^(-1) linewidth gives a gas to luminosity ratio M_(HI)/ L_V ≤ 2.6 × 10^(-2) M_⊙ L_⊙^(-1). The limits on H I mass and M_(HI)/L_V are typical of dwarf galaxies found within a few hundred kpc of the Milky Way. Whatever the origin of Hydra II, its neutral gas properties are not unusual.
Additional Information
© ESO, 2015. Received 8 September 2015 / Accepted 27 October 2015. We thank K. Spekkens for useful discussions and Richard Prestage for comments on the manuscript. These measurements were performed as part of the 2015 NRAO/NAIC Single Dish Summer School program.Attached Files
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Additional details
- Eprint ID
- 63718
- Resolver ID
- CaltechAUTHORS:20160115-125714532
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2016-01-19Created from EPrint's datestamp field
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2021-11-10Created from EPrint's last_modified field