TY - JOUR
T1 - Discovery and follow-up of a nearby galaxy from the Arecibo zone of avoidance survey
AU - McIntyre, T. P.
AU - Minchin, R. F.
AU - Momjian, E.
AU - Henning, P. A.
AU - Kaur, A.
AU - Parton, B.
PY - 2011/9/20
Y1 - 2011/9/20
N2 - The Arecibo L-Band Feed Array Zone of Avoidance (ALFA ZOA) Survey has discovered a nearby galaxy, ALFA ZOA J1952+1428, at a heliocentric velocity of +279km s-1. The galaxy was discovered at low Galactic latitude by 21cm emission from neutral hydrogen (H I). We have obtained follow-up observations with the Expanded Very Large Array and the 0.9m Southeastern Association for Research in Astronomy optical telescope. The H I distribution overlaps an uncataloged, potential optical counterpart. The H I linear size is 1.4kpc at our adopted distance of D = 7Mpc, but the distance estimate is uncertain as Hubble's law is unreliable at low recessional velocities. The optical counterpart has mB = 16.9mag and B - R = 0.1mag. These characteristics, including = 107.0 M⊙ and L B = 107.5 L⊙, if at 7Mpc, indicate that this galaxy is a blue compact dwarf, but this remains uncertain until further follow-up observations are complete. Optical follow-up observations are ongoing and near-infrared follow-up observations have been scheduled.
AB - The Arecibo L-Band Feed Array Zone of Avoidance (ALFA ZOA) Survey has discovered a nearby galaxy, ALFA ZOA J1952+1428, at a heliocentric velocity of +279km s-1. The galaxy was discovered at low Galactic latitude by 21cm emission from neutral hydrogen (H I). We have obtained follow-up observations with the Expanded Very Large Array and the 0.9m Southeastern Association for Research in Astronomy optical telescope. The H I distribution overlaps an uncataloged, potential optical counterpart. The H I linear size is 1.4kpc at our adopted distance of D = 7Mpc, but the distance estimate is uncertain as Hubble's law is unreliable at low recessional velocities. The optical counterpart has mB = 16.9mag and B - R = 0.1mag. These characteristics, including = 107.0 M⊙ and L B = 107.5 L⊙, if at 7Mpc, indicate that this galaxy is a blue compact dwarf, but this remains uncertain until further follow-up observations are complete. Optical follow-up observations are ongoing and near-infrared follow-up observations have been scheduled.
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U2 - 10.1088/2041-8205/739/1/L26
DO - 10.1088/2041-8205/739/1/L26
M3 - Article
AN - SCOPUS:80053487641
SN - 2041-8205
VL - 739
JO - Astrophysical Journal Letters
JF - Astrophysical Journal Letters
IS - 1
M1 - L26
ER -