A new CO bipolar flow and dense disk system associated with the infrared reflection nebula GGD 27 IRS

1989 ◽  
Vol 347 ◽  
pp. 894 ◽  
Author(s):  
Takuya Yamashita ◽  
Hiroko Suzuki ◽  
Norio Kaifu ◽  
Motohide Tamura ◽  
Charles M. Mountain ◽  
...  
1992 ◽  
Vol 389 ◽  
pp. 357 ◽  
Author(s):  
Joel H. Kastner ◽  
David A. Weintraub ◽  
C. Aspin

1988 ◽  
Vol 233 (4) ◽  
pp. 899-905
Author(s):  
T. Yamashita ◽  
S. Sato ◽  
M. Tamura ◽  
H. Suzuki ◽  
I. Gatley ◽  
...  

1986 ◽  
Vol 300 ◽  
pp. 406 ◽  
Author(s):  
M. W. Castelaz ◽  
J. A. Hackwell ◽  
G. L. Grasdalen ◽  
R. D. Gehrz

1995 ◽  
Vol 440 ◽  
pp. 722 ◽  
Author(s):  
T. J. T. Moore ◽  
T. Yamashita

1987 ◽  
Vol 225 (2) ◽  
pp. 393-398 ◽  
Author(s):  
I. S. McLean ◽  
M. J. McCaughrean ◽  
I. Gatley ◽  
J. Hough ◽  
S. Sato ◽  
...  

1994 ◽  
Vol 140 ◽  
pp. 270-271
Author(s):  
Karl R. Stapelfeldt

SVS 12 is an embedded infrared source which is the probable exciting star for HH 12. The source has a “class I” IRAS spectrum and about 20 L© luminosity. Differential reddening between the star (J-K ≥ 6 mag) and the adjacent infrared reflection nebula (J-K= 3 mag) suggests the presence of dense circumstellar material (Stapelfeldt et al. 1991). SVS 12 was observed with the OVRO interferometer in the 13CO 1-0 and CS 2-1 lines and associated continuum, and at the CSO with a bolometer and in the CS 5-4 and CS 7-6 lines.


1987 ◽  
Vol 314 ◽  
pp. 317 ◽  
Author(s):  
Michael W. Castelaz ◽  
John A. Hackwell

1985 ◽  
Vol 97 ◽  
pp. 924 ◽  
Author(s):  
M. W. Castelaz ◽  
R. D. Gehrz ◽  
G. L. Grasdalen ◽  
J. A. Hackwell

1986 ◽  
Vol 301 ◽  
pp. 502 ◽  
Author(s):  
Michael W. Castelaz ◽  
John A. Hackwell ◽  
Gary L. Grasdalen ◽  
Robert D. Gehrz ◽  
Craig Gullixson

1985 ◽  
Vol 290 ◽  
pp. 261 ◽  
Author(s):  
M. W. Castelaz ◽  
J. A. Hackwell ◽  
G. L. Grasdalen ◽  
R. D. Gehrz ◽  
C. Gullixson

Sign in / Sign up

Export Citation Format

Share Document