2010MNRAS.409.1412G

Query : 2010MNRAS.409.1412G

2010MNRAS.409.1412G - Mon. Not. R. Astron. Soc., 409, 1412-1428 (2010/December-3)

The JCMT Legacy Survey of the Gould Belt: a first look at Serpens with HARP.

GRAVES S.F., RICHER J.S., BUCKLE J.V., DUARTE-CABRAL A., FULLER G.A., HOGERHEIJDE M.R., OWEN J.E., BRUNT C., BUTNER H.M., CAVANAGH B., CHRYSOSTOMOU A., CURTIS E.I., DAVIS C.J., ETXALUZE M., DI FRANCESCO J., FRIBERG P., FRIESEN R.K., GREAVES J.S., HATCHELL J., JOHNSTONE D., MATTHEWS B., MATTHEWS H., MATZNER C.D., NUTTER D., RAWLINGS J.M.C., ROBERTS J.F., SADAVOY S., SIMPSON R.J., TOTHILL N.F.H., TSAMIS Y.G., VITI S., WARD-THOMPSON D., WHITE G.J., WOUTERLOOT J.G.A. and YATES J.

Abstract (from CDS):

The Gould Belt Legacy Survey on the James Clerk Maxwell Telescope's has observed a region of 260 arcmin2 in 12CO J= 3 -> 2 emission, and a 190 arcmin2 subset of this in 13CO and C18O towards the Serpens molecular cloud. We examine the global velocity structure of the non-outflowing gas, and calculate excitation temperatures and opacities. The large-scale mass and energetics of the region are evaluated, with special consideration for high-velocity gas. We find the cloud to have a mass of 203 M☉, and to be gravitationally bound, and that the kinetic energy of the outflowing gas is approximately 70 per cent of the turbulent kinetic energy of the cloud. We identify compact outflows towards some of the submillimetre Class 0/I sources in the region.

Abstract Copyright: 2010 The Authors. Monthly Notices of the Royal Astronomical Society2010 RAS

Journal keyword(s): molecular data - stars: formation - ISM: jets and outflows - ISM: kinematics and dynamics - submillimetre: ISM

Simbad objects: 21

goto Full paper

goto View the references in ADS

Number of rows : 21
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
2 NAME Ori B MoC 05 41 43.0 -01 54 44           ~ 1498 0
3 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
4 HH 106 HH 18 29 18.8 +01 14 17           ~ 15 0
5 HH 460 HH 18 29 38.6 +01 18 24           ~ 11 1
6 SH 2-68 N Y*O 18 29 48.09 +01 16 45.0           ~ 161 1
7 NAME Serpens Cloud SFR 18 29 49 +01 14.8           ~ 1195 1
8 GCNM 23 Y*O 18 29 49.63 +01 15 21.9           ~ 291 2
9 V* V371 Ser Or* 18 29 51.21240 +01 16 39.4860           ~ 132 1
10 [CED93] 7 smm 18 29 55.6 +01 14 52           ~ 4 0
11 [HCP2006] Cluster A Cld 18 29 56 +01 14.8           ~ 50 0
12 NAME Serpens SMM 4 cor 18 29 57.1 +01 13 15           ~ 143 0
13 IRAS 18274+0112 Y*O 18 29 57.73680 +01 14 05.6940           M4: 143 2
14 HH 458 HH 18 29 58.02 +01 13 43.2           ~ 5 1
15 NAME SERPENS SMM 3 Y*O 18 29 59.28 +01 14 01.7           ~ 111 1
16 NAME Serpens SMM 11 smm 18 30 00.3 +01 11 42           ~ 25 0
17 JCMTSE J183000.2+011251 Y*O 18 30 00.4 +01 12 50           ~ 53 0
18 [CED93] 8 smm 18 30 01.8 +01 15 07           ~ 18 0
19 HH 459 HH 18 30 02.6 +01 14 45           ~ 7 1
20 HD 170634 Or* 18 30 24.8757877680 +01 13 23.641855860 10.53 10.43 9.85     B8V 60 1
21 NAME Gould Belt PoG ~ ~           ~ 956 1

To bookmark this query, right click on this link: simbad:objects in 2010MNRAS.409.1412G and select 'bookmark this link' or equivalent in the popup menu