arXiv Analytics

Sign in

arXiv:1511.05069 [astro-ph.GA]AbstractReferencesReviewsResources

Limits on the HI content of the dwarf galaxy Hydra II

Andrew Janzen, Eve M. Klopf, Felix J. Lockman, Rodolfo Montez Jr, Kurt Plarre, Nau Raj Pokhrel, Robert J. Selina, A. Togi, Mehrnoush Zomederis

Published 2015-11-16Version 1

Sensitive 21cm HI 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 5-sigma limit of MHI < 210 solar masses for a 15 km/s linewidth gives a gas-to-luminosity ratio MHI/L_V < 2.6 x 10^{-2} Mo / Lo. The limits on HI mass and MHI/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.

Comments: Accepted for publication in Astronomy & Astrophysics
Categories: astro-ph.GA
Related articles: Most relevant | Search more
arXiv:1604.08862 [astro-ph.GA] (Published 2016-04-29)
The HI Content of Galaxies in Groups and Clusters as Measured by ALFALFA
arXiv:1411.0691 [astro-ph.GA] (Published 2014-11-03)
Search for PAHs in the Perseus molecular cloud with the Green Bank Telescope
arXiv:1605.01306 [astro-ph.GA] (Published 2016-05-04)
The Search for HI Emission at z $\approx0.4$ in Gravitationally Lensed Galaxies with the Green Bank Telescope