Xestia ursae

 
National Institutes of Health

Topic mentions per year

Topic mentions per year

1981-2004
01219812004

Papers overview

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2004
2004
We present spectroscopic observations of the short-period cataclysmic variable SW UMa obtained by the Far Ultraviolet… (More)
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2002
2002
Precise Doppler velocity measurements during 13 yr at Lick Observatory reveal the presence of two planets orbiting the star 47… (More)
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2000
2000
We present the first UBV anduvby photometric observations for the short period variable star HV Ursae Majoris classified as a… (More)
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1999
1999
The binary star BE Ursae Majoris is recently emerged from the common envelope phase ; indeed, the hot sdO/DAO component is the… (More)
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1999
1999
  • CH Ursae Majoris, Vojt ěchŠimon
  • 1999
An analysis of the historical light curve of the dwarf nova CH UMa, spanning 25 years, is presented. The statistical distribution… (More)
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1998
1998
We present new longitudinal magnetic field and Strömgren photometric measurements 1 of the Bp star 84 UMa. From these data we… (More)
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1998
1998
We observed the midand far-infrared spectral energy distributions of 9 A-type stars from the 300 Myrs old Ursae Majoris group… (More)
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1984
1984
As cataclysmic variables, SU Ursae Majoris stars1,2 are short-period binary systems consisting of a red dwarf star that fills its… (More)
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1983
1983
Among low luminosity galactic X-ray sources, AM Herculis-type binaries form a distinct class. The main characteristics of this… (More)
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1981
1981
BE Ursae Majoris is a 15-mag variable star of period 2.29 days, with a sinusoidal light curve of ∼1 mag amplitude1. Recently… (More)
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