Period-luminosity relations of variable stars in the Magellanic Clouds

Details Period-luminosity relations of variable stars in the Magellanic Clouds Period-luminosity relations of variable stars in the Magellanic Clouds

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asthe..98..163i&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 98, No. 3, p. 163 - 168 (2005)

Astronomy and Astrophysics

Astronomy

1

Magellanic Clouds, Variables, Period-Luminosity Relation

Scientific paper

We have performed a cross-identification between OGLE-II data and SIRIUS
near-infrared (NIR) JHK survey data in the Large and Small Magellanic
Clouds. Based on these homogeneous data, we studied the pulsation
properties and metallicity effects on period-K magnitude (PK) relations
by comparing the variable stars in the LMC and SMC.

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