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

scholarly journals THE INFLUENCE OF FAR-ULTRAVIOLET RADIATION ON THE PROPERTIES OF MOLECULAR CLOUDS IN THE 30 DOR REGION OF THE LARGE MAGELLANIC CLOUD

2009 ◽  
Vol 703 (1) ◽  
pp. 736-751 ◽  
Author(s):  
Jorge L. Pineda ◽  
Jürgen Ott ◽  
Ulrich Klein ◽  
Tony Wong ◽  
Erik Muller ◽  
...  
Keyword(s):  
Ultraviolet Radiation ◽  
Molecular Clouds ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Far Ultraviolet

scholarly journals [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of the Supernova Remnant N49 in the Large Magellanic Cloud

2000 ◽  
Vol 538 (1) ◽  
pp. L61-L64 ◽  
Author(s):  
William P. Blair ◽  
Ravi Sankrit ◽  
Robin Shelton ◽  
Kenneth R. Sembach ◽  
H. Warren Moos ◽  
...  
Keyword(s):  
Supernova Remnant ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Far Ultraviolet

scholarly journals CO in the Large Magellanic Cloud

1984 ◽  
Vol 108 ◽  
pp. 401-402 ◽  
Author(s):  
R. Cohen ◽  
J. Montani ◽  
M. Rubio
Keyword(s):  
Star Formation ◽  
Molecular Clouds ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Gas Content ◽  
Previous Survey ◽  
Interstellar Gas

In our galaxy molecular clouds account for about half the total interstellar gas and are probably the sites of all star formation. The high gas content and widespread star formation in the Large Magellanic Cloud would therefore suggest a high molecular content. Very little however is actually known about molecules in the LMC. The most extensive previous survey (see Israel in this volume) found CO in half of the 22 points observed but covered less than 10−4 of the LMC area.

Far-Ultraviolet Imaging of the Field Star Population in the Large Magellanic Cloud with the [ITAL]Hubble Space Telescope[/ITAL]

1999 ◽  
Vol 117 (1) ◽  
pp. 206-224 ◽  
Author(s):  
Noah Brosch ◽  
Michael Shara ◽  
John MacKenty ◽  
David Zurek ◽  
Brian McLean
Keyword(s):  
Hubble Space Telescope ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Space Telescope ◽  
Field Star ◽  
Far Ultraviolet

scholarly journals Far-Ultraviolet Imaging of the Large Magellanic Cloud Populous Cluster NGC 1978 with WFPC2

1997 ◽  
Vol 114 ◽  
pp. 1945 ◽  
Author(s):  
Andrew A. Cole ◽  
Jeremy R. Mould ◽  
John S., III Gallagher ◽  
John T. Clarke ◽  
John T. Trauger ◽  
...  
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Far Ultraviolet

scholarly journals Observations of O vi Absorption from the Superbubbles of the Large Magellanic Cloud

2013 ◽  
Vol 9 (S296) ◽  
pp. 388-389
Author(s):  
Ananta C. Pradhan ◽  
Amit Pathak ◽  
Jayant Murthy ◽  
D. K. Ojha
Keyword(s):  
Column Density ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Hot Gas ◽  
Far Ultraviolet

AbstractWe have presented the observations of O VI absorption at 1032 Å towards 22 sightlines in 10 superbubbles (SBs) of the Large Magellanic Cloud (LMC) using the data obtained from the Far Ultraviolet Spectroscopic Explorer (FUSE). The estimated abundance of O VI in the SBs varies from a minimum of (1.09 ±0.22)×1014 atoms/cm2 in SB N206 to a maximum of (3.71±0.23)×1014 atoms/cm2 in SB N70. We find about a 46% excess in the abundance of O VI in the SBs compared to the non-SB lines of sight. Even inside a SB, O VI column density (N(O VI)) varies by about a factor of 2 to 2.5. These data are useful in understanding the nature of the hot gas in SBs.

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 FAR-ULTRAVIOLET DIFFUSE EMISSION FROM THE LARGE MAGELLANIC CLOUD

2010 ◽  
Vol 718 (2) ◽  
pp. L141-L144 ◽  
Author(s):  
Ananta C. Pradhan ◽  
Amit Pathak ◽  
Jayant Murthy
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Diffuse Emission ◽  
Far Ultraviolet
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