scholarly journals Discovery of Shocked Molecular Clouds Associated with the Shell-type Supernova Remnant RX J0046.5−7308 in the Small Magellanic Cloud

2019 ◽  
Vol 881 (1) ◽  
pp. 85 ◽  
Author(s):  
H. Sano ◽  
H. Matsumura ◽  
Y. Yamane ◽  
P. Maggi ◽  
K. Fujii ◽  
...  
1995 ◽  
Vol 275 (4) ◽  
pp. 1218-1222 ◽  
Author(s):  
T. S. Ye ◽  
S. W. Amy ◽  
Q. D. Wang ◽  
L. Ball ◽  
J. Dickel

1991 ◽  
Vol 148 ◽  
pp. 429-430
Author(s):  
Monica Rubio

We summarize the results of observations of molecular gas from the Small Magellanic Cloud (SMC) made with low angular resolution (8'.8). These observations show that the CO emission is weak (TA˜ 0.04K) and that the CO luminosities of the Clouds are low compared to those of Galactic molecular clouds. The factor to convert the CO luminosity to molecular hydrogen column density for the SMC is ˜20 and three times larger than those derived for clouds in our Galaxy and in the Large Magellanic Cloud (LMC) respectively. In addition, we present preliminary results of high resolution (40″) observations of SMC molecular clouds made with the SEST telescope.


2014 ◽  
Vol 148 (5) ◽  
pp. 99 ◽  
Author(s):  
E. J. Crawford ◽  
M. D. Filipović ◽  
R. L. McEntaffer ◽  
T. Brantseg ◽  
K. Heitritter ◽  
...  

2010 ◽  
Vol 524 ◽  
pp. A52 ◽  
Author(s):  
C. Bot ◽  
M. Rubio ◽  
F. Boulanger ◽  
M. Albrecht ◽  
A. Leroy ◽  
...  

2003 ◽  
Vol 598 (2) ◽  
pp. L95-L98 ◽  
Author(s):  
Sangwook Park ◽  
John P. Hughes ◽  
David N. Burrows ◽  
Patrick O. Slane ◽  
John A. Nousek ◽  
...  

1989 ◽  
Vol 338 ◽  
pp. 812 ◽  
Author(s):  
William P. Blair ◽  
John C. Raymond ◽  
John Danziger ◽  
Francesca Matteucci

2011 ◽  
Vol 530 ◽  
pp. A132 ◽  
Author(s):  
R. A. Owen ◽  
M. D. Filipović ◽  
J. Ballet ◽  
F. Haberl ◽  
E. J. Crawford ◽  
...  

2011 ◽  
Vol 420 (1) ◽  
pp. L13-L17 ◽  
Author(s):  
V. Hénault-Brunet ◽  
L. M. Oskinova ◽  
M. A. Guerrero ◽  
W. Sun ◽  
Y.-H. Chu ◽  
...  

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