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_0 ~ 25. We also use narrowband H-alpha imaging from the KPNO 2.1-m
telescope to identify an HII 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.
Description
[1305.0270] ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. II. Optical Imaging Observations
cite arxiv:1305.0270Comment: 11 pages, 6 figures, 2 tables; published in The Astronomical Journal. Online AJ version at http://iopscience.iop.org/1538-3881/145/6/149/
%0 Generic
%1 rhode2013alfalfa
%A Rhode, Katherine L.
%A Salzer, John J.
%A Haurberg, Nathalie C.
%A Van Sistine, Angela
%A Young, Michael D.
%A Haynes, Martha P.
%A Giovanelli, Riccardo
%A Cannon, John M.
%A Skillman, Evan D.
%A McQuinn, Kristen B. W.
%A Adams, Elizabeth A. K.
%D 2013
%K HI dwarf galaxy
%T ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. II. Optical
Imaging Observations
%U http://arxiv.org/abs/1305.0270
%X 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_0 ~ 25. We also use narrowband H-alpha imaging from the KPNO 2.1-m
telescope to identify an HII 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.
@misc{rhode2013alfalfa,
abstract = {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_0 ~ 25. We also use narrowband H-alpha imaging from the KPNO 2.1-m
telescope to identify an HII 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.},
added-at = {2013-05-03T05:16:24.000+0200},
author = {Rhode, Katherine L. and Salzer, John J. and Haurberg, Nathalie C. and Van Sistine, Angela and Young, Michael D. and Haynes, Martha P. and Giovanelli, Riccardo and Cannon, John M. and Skillman, Evan D. and McQuinn, Kristen B. W. and Adams, Elizabeth A. K.},
biburl = {https://www.bibsonomy.org/bibtex/23276dd6eeb73580defb55f78ad1c7956/miki},
description = {[1305.0270] ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. II. Optical Imaging Observations},
interhash = {df232e39583cae2432c2fdb94cbfdd09},
intrahash = {3276dd6eeb73580defb55f78ad1c7956},
keywords = {HI dwarf galaxy},
note = {cite arxiv:1305.0270Comment: 11 pages, 6 figures, 2 tables; published in The Astronomical Journal. Online AJ version at http://iopscience.iop.org/1538-3881/145/6/149/},
timestamp = {2013-05-03T05:16:25.000+0200},
title = {ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. II. Optical
Imaging Observations},
url = {http://arxiv.org/abs/1305.0270},
year = 2013
}