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19982009
most citedThe mass and radius of the M-dwarf in the short period eclipsing binary RR Caeli

58 citations · 196 across the 11 of their papers we have counts for

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21 papers · 1 filter

astro-ph2008

Optical identification of a new cataclysmic variable from integral all sky survey: IGR J08390--4833

M. Revnivtsev, A. Kniazev, S. Sazonov +6

We have optically identified a recently discovered INTEGRAL source, IGR J08390--4833, with a cataclysmic variable, i.e. an accreting white dwarf in a binary system. The spectrum ex…

astro-ph200833 cited

Discovery of a massive variable star with Z=Zo/36 in the galaxy DDO 68

S. A. Pustilnik, A. L. Tepliakova, A. Y. Kniazev +1

The Local Volume dwarf galaxy DDO 68, from the spectroscopy of its two brightest HII regions (Knots 1 and 2) was designated as the second most metal-poor star-forming galaxy [12+lo…

astro-ph200824 cited

Estimating the birth period of pulsars through GLAST/LAT observations of their wind nebulae

O. C. de Jager

In this paper we show that the high energy -ray flux in the GeV domain from mature pulsar wind nebulae (PWN) scales as the change in rotational kinetic energy s…

astro-ph200820 cited

Spatially Resolved Imaging at 350um of Cold Dust in Nearby Elliptical Galaxies

Lerothodi L. Leeuw, Jacqueline Davidson, C. Darren Dowell +1

Continuum observations at 350um are presented of seven nearby elliptical galaxies, for which CO-gas disks have recently been resolved with interferometry mapping. These SHARCII map…

astro-ph20077 cited

Andromeda IV: a new Local Volume very metal-poor galaxy

S. A. Pustilnik, A. L. Tepliakova, A. Y. Kniazev +2

And IV is a low-surface brightness (LSB) dwarf galaxy at the distance of 6.1 Mpc, projecting close to M 31. In this paper the results of spectroscopy of And IV the two brightest HI…

astro-ph200714 cited

Keck spectroscopy and Spitzer Space Telescope analysis of the outer disk of the Triangulum Spiral Galaxy M33

David L. Block, Francoise Combes, Ivanio Puerari +11

In an earlier study of the spiral galaxy M33, we photometrically identified arcs or outer spiral arms of intermediate age (0.6 Gyr - 2 Gyr) carbon stars precisely at the commenceme…