... Mike Dopita's . HII Regions in Galaxies . LMC . SMC . NGC1313 . NGC1398 . ... NGC6744 . NGC247 . SNR 0102-72.3 in the SMC . SNR N132D in the LMC . NGC 2992. ...
... Elemental Abundance Patterns in the LMC Field Population around NGC 1846". ... The Large Magellanic Cloud (LMC) is an excellent candidate for this type of study ... of ~80 red giant stars around star cluster NGC 1846, located in the disc of the LMC ...
... Ca II triplet line strength measurements of LMC red giants that have high dispersion measurements of both [Fe/H] and [Ca/Fe] are used to investigate this question, noting that the LMC stars have quite different [Ca/Fe] from the Galactic calibration ...
... in distance modulus between the two nearby galaxies the Large Magellanic Cloud (LMC)and the Small Magellanic Cloud (SMC ... Then, assuming the distance to the LMC is 51 kpc, calculate the distance to the SMC. ...
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Ссылки http://www.mso.anu.edu.au/~wood/lectures2009/astr3007_ass3.pdf -- 49.4 Кб -- 31.03.2009 Похожие документы
... Galactic, LMC and SMC abundance patterns are used in a comparison of dusty and dust free models. ... We present results for [OIII] 5007 and [NII] 6583$lines for galactic, LMC and SMC abundances. Keywords . ...
... MSX sources in the LMC: Dust-enshrouded AGB stars, post-AGB stars and PN . ... MSX sources in the LMC: dust-enshrouded AGB stars and post-AGB stars . ... Variable Red Giants in the LMC: Pulsating Stars and Binaries? ...