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Frontal margin of sphenoid

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

Papers overview

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2016
2016
We report that the spectroscopic binary μ Ursae Majoris (μ UMa) has secondary RV variations of 471.2 days in addition to those of… Expand
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2015
2015
With extensive sets of new radial velocities we have determined orbital elements for three previously known spectroscopic… Expand
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Review
2010
Review
2010
We present the first pointed X-ray observation of DW Ursae Majoris, a novalike cataclysmic variable (CV) and one of the archetype… Expand
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Highly Cited
2007
Highly Cited
2007
For the past 3 years we have been monitoring a sample of 62 K giant stars using precise stellar radial velocity measurements with… Expand
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2005
2005
We numerically investigated the dynamical architecture of 47 UMa with the planetary configuration of the best-fit orbital… Expand
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2004
2004
Received ;accepted Abstract. We present an analysis of CCD photometric observations of the eclipsing novalike cataclysmic… Expand
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2002
2002
We have investigated whether Earth-mass planets could survive in the habitable zone (HZ) of the 47 Ursae Majoris system. Mixed… Expand
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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… Expand
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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… Expand