SPLASH: the Southern Parkes Large-Area Survey in Hydroxyl - first science from the pilot region

被引:41
作者
Dawson, J. R. [1 ,2 ]
Walsh, A. J. [3 ]
Jones, P. A. [4 ]
Breen, S. L. [1 ]
Cunningham, M. R. [4 ]
Lowe, V. [1 ,4 ]
Jones, C. [1 ,2 ]
Purcell, C. [5 ]
Caswell, J. L. [1 ]
Carretti, E. [1 ]
McClure-Griffiths, N. M. [1 ]
Ellingsen, S. P. [2 ]
Green, J. A. [1 ,6 ]
Gomez, J. F. [7 ]
Krishnan, V. [1 ,2 ]
Dickey, J. M. [2 ]
Imai, H. [8 ]
Gibson, S. J. [9 ]
Hennebelle, P. [10 ,11 ]
Lo, N. [12 ]
Hayakawa, T. [13 ]
Fukui, Y. [13 ]
Mizuno, A. [14 ]
机构
[1] CSIRO Astron & Space Sci, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[2] Univ Tasmania, Sch Math & Phys, Hobart, Tas 7000, Australia
[3] Curtin Univ, Int Ctr Radio Astron Res, Perth, WA 6845, Australia
[4] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia
[5] Univ Sydney, Sch Phys, Sydney Inst Astron SiFA, Sydney, NSW 2006, Australia
[6] SKA Org, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[7] Inst Astrofis Andalucia CSIC, E-18080 Granada, Spain
[8] Kagoshima Univ, Dept Phys & Astron, Grad Sch Sci & Engn, Kagoshima 8900065, Japan
[9] Western Kentucky Univ, Dept Phys & Astron, Bowling Green, KY 42101 USA
[10] Ecole Normale Super, Lab Radioastron, F-75231 Paris 05, France
[11] CNRS, Observ Paris, UMR 8112, F-75231 Paris 05, France
[12] Univ Chile, Dept Astron, Santiago, Chile
[13] Nagoya Univ, Dept Phys & Astrophys, Chikusa Ku, Nagoya, Aichi 4648601, Japan
[14] Nagoya Univ, Solar Terr Environm Lab, Chikusa Ku, Nagoya, Aichi 4648601, Japan
基金
澳大利亚研究理事会;
关键词
masers; surveys; ISM: molecules; Galaxy: disc; radio lines: ISM; INTERSTELLAR DUST CLOUDS; STAR-FORMING REGIONS; EMISSION-ABSORPTION OBSERVATIONS; NARROW SELF-ABSORPTION; GHZ METHANOL MASERS; 1612 MHZ SURVEY; ALL-SKY SURVEY; OH-EMISSION; GALACTIC OH; MOLECULAR CLOUDS;
D O I
10.1093/mnras/stu032
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Southern Parkes Large-Area Survey in Hydroxyl (SPLASH) is a sensitive, unbiased, and fully sampled survey of the southern Galactic plane and Galactic Centre in all four ground-state transitions of the hydroxyl (OH) radical. The survey provides a deep census of 1612-, 1665-, 1667-, and 1720-MHz OH absorption and emission from the Galactic interstellar medium, and is also an unbiased search for maser sources in these transitions. We present here first results from the SPLASH pilot region, which covers Galactic longitudes 334 degrees to 344 degrees and latitudes +/- 2 degrees. Diffuse OH is widely detected in all four transitions, with optical depths that are always small (averaged over the Parkes beam), and with departures from local thermodynamic equilibrium common even in the 1665- and 1667-MHz main lines. To a 3 Sigma sensitivity of similar to 30 mK, we find no evidence of OH envelopes extending beyond the CO-bright regions of molecular cloud complexes, and conclude that the similarity of the OH excitation temperature and the level of the continuum background is at least partly responsible for this. We detect masers and maser candidates in all four transitions, approximately 50 per cent of which are new detections. This implies that SPLASH will produce a substantial increase in the known population of ground-state OH masers in the southern Galactic plane.
引用
收藏
页码:1596 / 1614
页数:19
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