Other
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20919201g&link_type=abstract
2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #192.01; Bulletin of the American Astronomical Society,
Other
Scientific paper
The LMC is unusual in that its history and properties have been affected by its close proximity to the Milky Way and interactions with the SMC. Yet in many ways, such as the structure of its main stellar body and chemical abundance patterns, the LMC also is a fairly normal example of a moderate luminosity disk galaxy. Because the LMC is nearby with little extinction and a low inclination, it remains the best studied galaxy other than the Milky Way. In the spirit of our program, Surveying the Agents of a Galaxy's Evolution (SAGE), this talk charts the locations and parameters of major baryonic components of the LMC, ISM and stars, and briefly summarizes the history of star formation in the LMC. The state of the LMC's interstellar medium in relationship to the global structure of the galaxy and populations of recently formed stars is one of the primary topics of SAGE, and will be discussed with an emphasis on differences between conditions in the LMC and those in the Milky Way.
The SAGE Project is supported by NASA/Spitzer grant 1275598 and NASA NAG5-12595
Babler Brian
Bernard JP.
Block Martin M.
Blum Robert
Churchwell Edward
No associations
LandOfFree
The Large Magellanic Cloud as a Galaxy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Large Magellanic Cloud as a Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Large Magellanic Cloud as a Galaxy will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1163268