Frontal margin of sphenoid

Known as: Margo frontalis alaris majoris ossis sphenoidalis 
 
National Institutes of Health

Topic mentions per year

Topic mentions per year

1942-2017
0119422016

Papers overview

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2017
2017
X-ray observations throughout the orbital cycle of AN UMa during its low state were conducted with the Einstein Observatory… (More)
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2009
2009
In this Letter, the radial velocity variability of the chemically peculiar star ǫ Ursae Majoris (ǫ UMa) from the sharp cores of… (More)
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2008
2008
Well-determined physical parameters of 130 W UMa systems have been collected from the literature. Based on these data, the… (More)
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Review
2006
Review
2006
Because of the similarity of the primary star of HS 1136+6646 to the planetary nebula central star BE Ursae Majoris, we did wide… (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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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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1997
1997
Possible planetary objects have now been discovered1–9 orbiting nine different main-sequence stars. These companion objects (some… (More)
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1993
1993
ACCRETION disks play an important role in many astrophysical environments, such as active galactic nuclei, protostellar systems… (More)
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1991
1991
THE possibility of using an artificial 'guide-star' to measure optical wavefront distortion caused by atmospheric turbulence has… (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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