Far Ultraviolet Spectroscopic ExplorerObservations of Interstellar Gas toward the Small Magellanic Cloud Star Sk 108

2001 ◽  
Vol 558 (1) ◽  
pp. 133-144 ◽  
Author(s):  
C. Mallouris ◽  
D. E. Welty ◽  
D. G. York ◽  
H. W. Moos ◽  
K. R. Sembach ◽  
...  
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
Interstellar Gas ◽  
Far Ultraviolet

scholarly journals Ultraviolet Interstellar Absorption Towards SK159 in the Small Magellanic Cloud

1984 ◽  
Vol 108 ◽  
pp. 407-408
Author(s):  
Edward L. Fitzpatrick
Keyword(s):  
Signal To Noise Ratio ◽  
Magellanic Cloud ◽  
High Dispersion ◽  
Small Magellanic Cloud ◽  
Interstellar Gas ◽  
Stellar Spectrum ◽  
H Ii Region ◽  
Halo Gas ◽  
Marginal Detection ◽  
Great Complexity

Multiple high-dispersion IUE spectra of SK159 in the Small Magellanic Cloud (SMC) have been obtained and averaged in order to study interstellar gas associated with the SMC and, in particular, to search for evidence of SMC halo gas. A single high-dispersion IUE spectrum of SK159 was analyzed by Prévot et al. (1980). They reported the absence of C IV and only the marginal detection of Si IV at SMC velocities. The higher signal-to-noise ratio in our data allow a more definitive investigation of the absorption characteristics of these ions. SK159 is relatively cool, spectral type BO.5 Iaw (Walborn 1983) and is located in a region free of strong nebulosity. Thus the interstellar line spectrum will be less contaminated by H II region absorption than in previous studies of SMC stars. This favorable circumstance is somewhat offset by the great complexity of the underlying stellar spectrum and the resultant blending of stellar and interstellar lines.

scholarly journals Distribution of young stars and gas in the Small Magellanic Cloud

1991 ◽  
Vol 148 ◽  
pp. 25-29
Author(s):  
J. Lequeux
Keyword(s):  
Strong Evidence ◽  
Magellanic Cloud ◽  
Young Stars ◽  
Radial Velocities ◽  
Small Magellanic Cloud ◽  
Interstellar Gas

The relations between the distributions of interstellar gas and young stars in the central parts of the SMC are discussed, based on their distributions over the sky, radial velocities and distances. There are large differences between stars and gas. The existence of two main complexes is confirmed. There is no strong evidence for a distance in depth between these complexes larger than about 10 kpc, although Cepheid observations suggest a large total depth in some regions. Further, more accurate observations of Cepheids, especially of their mean radial velocities, are required for a better understanding of the structure of the SMC.

scholarly journals Far‐Ultraviolet and Hα Spectroscopy of SNR 0057−7226 in the Small Magellanic Cloud HiiRegion N66

2003 ◽  
Vol 586 (2) ◽  
pp. 1179-1190 ◽  
Author(s):  
Charles W. Danforth ◽  
Ravi Sankrit ◽  
William P. Blair ◽  
J. Christopher Howk ◽  
You‐Hua Chu
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
Far Ultraviolet

scholarly journals Far‐Ultraviolet and X‐Ray Observations of the Reverse Shock in the Small Magellanic Cloud Supernova Remnant 1E 0102.2−7219

2006 ◽  
Vol 642 (1) ◽  
pp. 260-269 ◽  
Author(s):  
Manami Sasaki ◽  
Terrance J. Gaetz ◽  
William P. Blair ◽  
Richard J. Edgar ◽  
Jon A. Morse ◽  
...  
Keyword(s):  
Supernova Remnant ◽  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
Reverse Shock ◽  
X Ray ◽  
Far Ultraviolet

scholarly journals OBSERVATIONS OF FAR-ULTRAVIOLET DIFFUSE EMISSION FROM THE SMALL MAGELLANIC CLOUD

2011 ◽  
Vol 743 (1) ◽  
pp. 80 ◽  
Author(s):  
Ananta C. Pradhan ◽  
Jayant Murthy ◽  
Amit Pathak
Keyword(s):  
Magellanic Cloud ◽  
Small Magellanic Cloud ◽  
Diffuse Emission ◽  
Far Ultraviolet

scholarly journals [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of Interstellar Gas toward the Large Magellanic Cloud Star S[CLC]k[/CLC] −67°05

2000 ◽  
Vol 538 (1) ◽  
pp. L39-L42 ◽  
Author(s):  
S. D. Friedman ◽  
J. C. Howk ◽  
B-G Andersson ◽  
K. R. Sembach ◽  
T. B. Ake ◽  
...  
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Interstellar Gas ◽  
Far Ultraviolet
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