... CSIROpedia . Workshop on Surveys and the ISM of the Galaxy and LMC . 19:00 Thu 17 Feb to 11:00 Fri 18 Feb 2005 . ... SESSION 3 (15:30 to 17:30) . THE ISM AND SURVEYS OF THE LMC [15 min talks] . <ul> . <li> A. Kawamura (Dark Clouds) . ...
... What do physical properties of the GCS of the LMC tell us about the LMC formation ... LMC GCS: V/~2.4 Halo: V/~0.2 GC Halo field stars LMC The non-rotating stellar halo ...
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Ссылки http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/LMC07a.pdf -- 813.1 Кб -- 04.08.2007 Похожие документы
... LMC, SMC, and a part of the Bridge · LMC 40 deg2 (3,249 fields) IRSF Zaritsky ... LMC bar IRSF FWHM: 2".6 Nsrc ~ 800 1".2 Nsrc ~ 3600 FWHM: Our higher resolution ... LMC; Ks) undetectable by 2MASS log10 N Tip of RGB red clump Features by T-RGB and RC ...
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Ссылки http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/australia070716.pdf -- 2601.0 Кб -- 04.08.2007 Похожие документы
... Oswego) ABSTRACT: We determine the LMC distance using Cepheid variables in the LMC ... LMC Cepheid distances obtained from the infrared surface brightness method and a ...
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Ссылки http://www.atnf.csiro.au/research/LVmeeting/posters/Ngeow.poster.pdf -- 189.1 Кб -- 25.06.2007 Похожие документы
... Results with the ATCA 3mm Prototype System (July 2001) . HCN(1-0) and HCO + (1-0) spectra of N159HW in the LMC, by Tony Wong. ... GHz. Uncalibrated HCN(1-0) and HCO + (1-0) emission spectra of N159HW in the LMC. ...