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most citedThe period-luminosity relation for type II Cepheids in globular clusters

94 citations · 233 across the 5 of their papers we have counts for

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astro-ph200882 cited

AGB Stars in the Fornax Dwarf Spheroidal Galaxy

Patricia A. Whitelock, John W. Menzies, Michael W. Feast +3

We report on a multi-epoch study of the Fornax dwarf spheroidal galaxy, made with the Infrared Survey Facility, over an area of about 42'x42'. The colour-magnitude diagram shows a…

astro-ph200854 cited

AKARI Near Infrared Spectroscopy: Detection of H2O and CO2 Ices toward Young Stellar Objects in the Large Magellanic Cloud

Takashi Shimonishi, Takashi Onaka, Daisuke Kato +4

We present the first results of AKARI Infrared Camera near-infrared spec- troscopic survey of the Large Magellanic Cloud (LMC). We detected absorption features of the H2O ice 3.05…

astro-ph200694 cited

The period-luminosity relation for type II Cepheids in globular clusters

Noriyuki Matsunaga, Hinako Fukushi, Yoshikazu Nakada +11

We report the result of our near-infrared observations (JHKs) for type II Cepheids (including possible RV Tau stars) in galactic globular clusters. We detected variations of 46 var…

astro-ph2004

Chemical composition of UV-bright star ZNG 4 in the globular cluster M13

S. Ambika, M. Parthasarathy, W. Aoki +4

We present a detailed model-atmosphere analysis of ZNG 4, a UV-bright star in the globular cluster M13. From the analysis of a high resolution () spectrum of th…

astro-ph2003

Variable stars in the Magellanic Clouds: II. The data and infrared properties

Yoshifusa Ita, Toshihiko Tanabe, Noriyuki Matsunaga +10

The data of 8,852 and 2,927 variable stars detected by OGLE survey in the Large and Small Magellanic Clouds are presented. They are cross-identified with the SIRIUS JHK survey data…

astro-ph2003

Variable Stars in the Magellanic Clouds: Results from OGLE and SIRIUS

Yoshifusa Ita, Toshihiko Tanabe, Noriyuki Matsunaga +10

We have performed a cross-identification between OGLE-II data and single-epoch SIRIUS JHK survey data in the LMC and SMC. After eliminating obvious spurious variables, we determine…