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19982004
most citedOptical Line profile variability of the B1+neutron star binary system LS I+65 010 = 2S 0114+650

4 citations · 4 across the 2 of their papers we have counts for

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astro-ph200736 cited

The enigma of the oldest `nova': the central star and nebula of CK Vul

M. Hajduk, Albert A. Zijlstra, P. A. M. van Hoof +9

CK Vul is classified as, amongst others, the slowest known nova, a hibernating nova, or a very late thermal pulse object. Following its eruption in AD 1670, the star remained visib…

astro-ph2004

Planetary Nebulae as Probes of the Chemical Evolution of Dynamically Hot Systems

Michael G. Richer, Marshall L. McCall

The measurement of chemical abundances in planetary nebulae in nearby galaxies is now relatively straightforward. The challenge is to use these chemical abundances to infer the che…

astro-ph20024 cited

Optical Line profile variability of the B1+neutron star binary system LS I+65 010 = 2S 0114+650

Gloria Koenigsberger, Gabriela Canalizo, Anabel Arrieta +2

We present high resolution spectroscopic observations of the massive X-ray binary system LS I+65 010=2S 0114+650 in the optical wavelength region. A correlation between equivalent…

astro-ph2000

The Red Stellar Contents of Three Selected Fields of The Local Group Dwarf Irregular Galaxy IC1613

J. Borissova, L. Georgiev, R. Kurtev +4

We present a moderately-deep JK photometry for three selected areas of the dwarf irregular galaxy IC1613. The color-magnitude diagrams contain a mixture of red supergiants, asympto…

astro-ph1998

The chemical evolution of dynamically hot galaxies

Michael G. Richer, Marshall L. McCall, Grazyna Stasinska

We investigate the chemical properties of M32, the bulges of M31 and the Milky Way, and the dwarf spheroidal galaxies NGC 205, NGC 185, Sagittarius, and Fornax using previously pub…