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Parietal margin of sphenoid

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

Papers overview

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2016
2016
We used the newly commissioned 50 cm Binocular Network (50BiN) telescope at Qinghai Station of Purple Mountain Observatory… 
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Review
2013
Review
2013
A nearby friable cloud in Ursa Majoris contains 270 galaxies with radial velocities 500 < VLG < 1500 km s^-1 inside the area of… 
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2011
2011
We report results of an extensive world-wide observing campaign devoted to the recently discovered dwarf nova SDSS J162520.29… 
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Review
2009
Review
2009
Parallaxes of W UMa stars in the Hipparcos catalogue have been analyzed. 31 W UMa stars, which have the most accurate parallaxes… 
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2008
2008
In this Letter, the radial velocity variability of the chemically peculiar star e Ursae Majoris (e UMa) from the sharp cores of… 
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Highly Cited
2000
Highly Cited
2000
We report the results of deep observations at radio (3.6 cm) wavelengths of the nearby solar-type star pi 01 Ursa Majoris with… 
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1999
1999
  • Gao, Li, Wu, Zhang
  • The Astrophysical journal
  • 1999
  • Corpus ID: 16090638
We report the photometry of a peculiar SU Ursae Majoris-type dwarf nova, ER Ursae Majoris, for 10 nights during 1998 December and… 
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1998
1998
We observed the mid- and far-infrared spectral en- ergy distributions of 9 A-type stars from the 300 Myrs old Ursae Majoris group… 
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1997
1997
We have used the Navy Prototype Optical Interferometer (NPOI) to obtain the first multichannel optical aperture synthesis images… 
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