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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… 
2015
2015
With extensive sets of new radial velocities we have determined orbital elements for three previously known spectroscopic… 
Review
2012
Review
2012
We report on a BVRCIC survey of field W Ursae Majoris binary stars and present accurate colors for 606 systems that have been… 
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… 
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… 
2004
2004
Received ;accepted Abstract. We present an analysis of CCD photometric observations of the eclipsing novalike cataclysmic… 
2002
2002
We have investigated whether Earth-mass planets could survive in the habitable zone (HZ) of the 47 Ursae Majoris system. Mixed… 
1999
1999
The binary star BE Ursae Majoris is recently emerged from the common envelope phase; indeed, the hot sdO/DAO component is the… 
Highly Cited
1998
Highly Cited
1998
We present a detailed analysis of two spectroscopic binaries based on new observations obtained with the Navy Prototype Optical…