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 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

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 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.

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

scholarly journals The Detection of Far‐Ultraviolet Line Emission from Balmer‐Dominated Supernova Remnants in the Large Magellanic Cloud

2007 ◽  
Vol 664 (1) ◽  
pp. 304-321 ◽  
Author(s):  
Parviz Ghavamian ◽  
William P. Blair ◽  
Ravi Sankrit ◽  
John C. Raymond ◽  
John P. Hughes
Keyword(s):  
Supernova Remnants ◽  
Line Emission ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
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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