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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3630
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dc.contributor.authorSagar, R-
dc.contributor.authorYu, Q. Z-
dc.date.accessioned2008-09-15T15:00:36Z-
dc.date.available2008-09-15T15:00:36Z-
dc.date.issued1990-04-
dc.identifier.citationAstrophysical Journal, Part 1, Vol. 353, No.1, pp. 174 - 180en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/3630-
dc.description.abstractThe JHK magnitudes of 29 stars in the region of open star cluster IC 1805 were measured. These, and the existing infrared and optical observations, indicate a normal interstellar extinction law in the direction of the cluster. Further, most of the early-type stars have near-infrared fluxes as expected from their spectral types. Patchy distribution of ionized gas and dust appears to be the cause of nonuniform extinction across the cluster face.en
dc.language.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://ads.iucaa.ernet.in/abs/1990ApJ...353..174Sen
dc.subjectInfrared photometryen
dc.subjectOpen clustersen
dc.subjectColor-color diagramen
dc.subjectEarly starsen
dc.subjectInfrared astronomy satelliteen
dc.subjectInterstellar extinctionen
dc.subjectIonized gasesen
dc.titleNear-infrared photometric study of open star cluster IC 1805en
dc.typeArticleen
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