... sources discovered in the Large Magellanic Cloud (LMC) by the MSX satellite in 1996 ... ordinary giant stars (small dots) and infrared MSX sources (large dots) in the LMC ...
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Ссылки http://www.mso.anu.edu.au/annualReport/2000/ann.rep.2000.pdf -- 1496.6 Кб -- 15.10.2004 Похожие документы
... check the Cepheid Period-Luminosity (PL) relation in the Large Magellanic Cloud (LMC ... observations of ~35 Cepheids and a standard distance to the LMC of 50 kiloparsecs ...
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Ссылки http://www.mso.anu.edu.au/annualReport/2001/annrep_2001.pdf -- 398.8 Кб -- 15.10.2004 Похожие документы
... Talk: "MACHO Observations of LMC Red Giants", Wood P R and the MACHO Collaboration. 3rd Torino Workshop: AGB Star Models and Observations, Grenoble, 3-5 September. ...
... which uses a distance modulus to the Large Magellanic Cloud (LMC) of 18.50 mag ... the Hipparcos satellite indicate that the LMC distance could be greater, and hence ... if one increases the distance to the LMC, the dynamical age of the universe ...
... Host: Sarah Sweet . Shaheen Iqbal (RSAA) . Elemental Abundance Patterns in the LMC Field Population around NGC 1846 . 07/05/2015, 11:00-12:00 . ...
... The maximum variation observed was LMC is 2.35 kpc and SMC is 3.2 kpc. ... DR2 takes its data from 936 fields. A 3D representation of the LMC and SMC. ... RR Lyrae Variables and the LMC Distance", Astronomical Journal, Vol 127, pp 334-354 ...
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Ссылки http://www.mso.anu.edu.au/annualReport/2004/RSAA_AR2004.pdf -- 1673.3 Кб -- 11.04.2006 Похожие документы
... We installed a 400 mm lens in front of a 2Kx2K CCD and using glass filters and interference filters have taken 7 degree images of the LMC and SMC in H alpha, [SII], [OIII] and continuum. ...
... K. H., Nikolaev, S., Huber, M., Prochtor, G., Clocchiatti, A., Minniti, D., Garg, A., Challis, P., Keller, S. C., Schmidt, B. P., 2005, ApJ, 634, 1103 "Testing LMC Microlensing Scenarios: The Discrimination Power of the SuperMACHO Microlensing Survey" 49 ...