... LMC planetary nebulae {PNe} in order to study the co-evolution of the nebulae and their central stars, and to probe the ... LMC distance remain controversial and uncertain to ~10-15, using eclipsing binaries {EBs} as "standard candles'' to include two ...
... Resolving the LMC Microlensing Puzzle: Where Are the Lensing Objects ? . Abstract . ... GO 10583: Resolving the LMC Microlensing Puzzle: Where Are the Lensing Objects ? ...
... Spitzer SAGE Survey of the LMC, an example This past decade ground based and space ... Spitzer Survey of the Large Magellanic Cloud (LMC): Surveying the Agents of a Galaxy ...
[
Текст
]
Ссылки http://www.stsci.edu/jwst/doc-archive/white-papers/JWST_stellar_pop.pdf -- 472.7 Кб -- 05.02.2013 Похожие документы
... High velocity components around 300 are located in front of the LMC main velocity layers at 245 and 280 which are also the large scale bodies of neutral hydrogen in this direction of the LMC. ...
... as of 130/0000Z 1.0 OBSERVATIONS SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 8702 (The Most Elusive Nuclei of LMC Planetary Nebulae) The WF/PC-2 was used to carry out a SNAPSHOT survey of the faintest nuclei of planetary nebulae {PNe} in the LMC ...
... Cepheids in the LMC: the original PLC . ... In the case of the Hubble H 0 Key Project, the LMC distance modulus is set at 18.5 ... using a variety of distance estimators give LMC distance molduli that range from 18 ...
... Resolving the LMC Microlensing Puzzle: Where Are the Lensing Objects ? . Abstract . ... The Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC) are the most ...