Hipass detection of an intergalactic gas cloud in the NGC 2442 group

被引:58
作者
Ryder, SD
Koribalski, B
Staveley-Smith, L
Kilborn, VA
Malin, DF
Banks, GD
Barnes, DG
Bhatal, R
de Blok, WJG
Boyce, PJ
Disney, MJ
Drinkwater, MJ
Ekers, RD
Freeman, KC
Gibson, BK
Henning, PA
Jerjen, H
Knezek, PM
Marquarding, M
Minchin, RF
Mould, JR
Oosterloo, T
Price, RM
Putman, ME
Sadler, EM
Stewart, I
Stootman, F
Webster, RL
Wright, AE
机构
[1] Anglo Australian Observ, Epping, NSW 1710, Australia
[2] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[3] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia
[4] Univ Wales, Dept Phys & Astron, Cardiff CF2 3YB, S Glam, Wales
[5] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[6] Univ Western Sydney Macarthur, Dept Phys, Campbelltown, NSW 2560, Australia
[7] Mt Stromlo & Siding Spring Observ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[8] Univ New Mexico, Dept Phys & Astron, Albuquerque, NM 87131 USA
[9] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[10] ASTRON, NL-7990 AA Dwingeloo, Netherlands
[11] Univ Sydney, Sch Phys A28, Sydney, NSW 2006, Australia
[12] Univ Leicester, Dept Phys & Astron, Xray Astron Grp, Leicester LE1 7RH, Leics, England
关键词
galaxies : individual (NGC 2442); galaxies : interactions; galaxies : intergalactic medium; radio lines : galaxies;
D O I
10.1086/321453
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery from the H I Parkes All-Sky Survey (HIPASS) of a gas cloud associated with the asymmetric spiral galaxy NGC 2442. This object, designated HIPASS J0731-69, contains similar to 10(9) M-. of H I, or nearly one-third as much atomic gas as NGC 2442 itself. No optical counterpart to any part of HIPASS J0731-69 has yet been identified, consistent with the gas being diffuse and its streamlike kinematics. If the gas in HIPASS J0731-69 was once part of NGC 2442, then it was most likely a fairly recent tidal encounter with a moderately massive companion that tore it loose, although the possibility of ram-pressure stripping cannot be ruled out. This discovery highlights the potential of the HIPASS data for yielding new clues to the nature of some of the best-known galaxies in the local universe.
引用
收藏
页码:232 / 239
页数:8
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