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19932020
most citedGalactic Kinematics of Cepheids from Hipparcos Proper Motions

320 citations · 3.4k across the 70 of their papers we have counts for

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70 papers

astro-ph.SR2020★ 11 cited

Light and colour variations of Mira variables in the Small Magellanic Cloud

Yoshifusa Ita, John W. Menzies, Patricia A. Whitelock +6

The goal of this paper is to characterise the light variation properties of Mira variables in the Small Magellanic Cloud. We have investigated a combined optical and near infrared…

astro-ph.SR2018★ 14 cited

Luminous AGB variables in the dwarf Irregular Galaxy, NGC 3109

J. W. Menzies, P. A. Whitelock, M. W. Feast +1

In a shallow near-infrared survey of the dwarf Irregular galaxy, NGC 3109, near the periphery of the Local Group, we have found eight Mira variables, seven of which appear to be ox…

astro-ph.SR2018★ 9 cited

R Coronae Borealis: Radial-velocity and other observations, 1950-2007

M. W. Feast, R. F. Griffin, G. H. Herbig +1

Radial-velocity observations made on more than a thousand nights are presented for the type star of the R Coronae Borealis (RCB) class. There are four principal sources: the Lick O…

astro-ph.SR2018★ 11 cited

A near infrared variable star survey in the Magellanic Clouds: The Small Magellanic Cloud data

Yoshifusa Ita, Noriyuki Matsunaga, Toshihiko Tanabe +12

A very long term near-infrared variable star survey towards the Large and Small Magellanic Clouds was carried out using the 1.4m InfraRed Survey Facility at the South African Astro…

astro-ph.GA2017★ 19 cited

A Remarkable Oxygen-rich Asymptotic Giant Branch Variable in the Sagittarius Dwarf Irregular Galaxy

Patricia A. Whitelock, John W. Menzies, Michael W. Feast +1

We report and discuss JHKs photometry for Sgr dIG, a very metal-deficient galaxy in the Local Group, obtained over 3.5 years with the Infrared Survey Facility in South Africa. Thre…

astro-ph.SR2017★ 25 cited

Discovery of carbon-rich Miras in the Galactic bulge

Noriyuki Matsunaga, John W. Menzies, Michael W. Feast +4

Only one carbon-rich (C-rich, hereinafter) Mira variable has so far been suggested as a member of the Galactic bulge and this is in a symbiotic system. Here we describe a method fo…