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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5423
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dc.contributor.authorSubramaniam, A-
dc.contributor.authorSubramanian, S-
dc.date.accessioned2011-03-17T14:55:53Z-
dc.date.available2011-03-17T14:55:53Z-
dc.date.issued2010-
dc.identifier.citationOjha, D. K., ed., Interstellar matter and star formation: a multi-wavelength Perspective, An international workshop held as part of the Homi Bhabha Birth Centenary Celebrations, Hyderabad, India Oct 5-7, 2009, pp. 107-110en
dc.identifier.isbn978-81-8465-441-7-
dc.identifier.urihttp://hdl.handle.net/2248/5423-
dc.descriptionRestricted Accessen
dc.description.abstractWe present the internal and foreground reddening maps of the Large and Small Magellanic Clouds. These are estimated using the red clump stars identified from the OGLE III catalog. The foreground reddening is estimated from the shift of the peak in the red clump colour distribution and the internal reddening from the width of the colour distribution, after correcting for population effects. The foreground reddening in the LMC is found to be correlated with the location of the star forming regions. The reddening towards the LMC is found to be larger than that towards the SMC.en
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.ispartofseriesASI Conference Series, Vol. 1-
dc.rights© Astronomical Society of Indiaen
dc.subjectMagellanic Cloudsen
dc.subjectRed clump starsen
dc.titleInternal and foreground reddening maps of the Magellanic Cloudsen
dc.typeArticleen
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