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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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2014
2014
OBJECTIVE To investigate the Daodi habitat of Panacis Majoris Rhizoma by analyzing the characteristics of inorganic elements in… 
Review
2012
Review
2012
A nearby friable cloud in Ursa Majoris contains 270 galaxies with radial velocities 500 < VLG < 1500 km s^-1 inside the area of… 
2011
2011
We report results of an extensive world-wide observing campaign devoted to the recently discovered dwarf nova SDSS J162520.29… 
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… 
1998
1998
Low amplitude (≃ 0.5%) 29-s oscillations have been detected in HST/FOS eclipse observations of the nova-like cataclysmic variable… 
1997
1997
Accurate stellar parameters are presented for the solar-type stars 51 Peg and 47 UMa. The announcement of the detection of jovian… 
1993
1993
ACCRETION disks play an important role in many astrophysical environments, such as active galactic nuclei, protostellar systems… 
1965
1965
IN a new development of the fission theory of the origin of close binary stars1,2, I showed that rotational instability would… 
1965
1965
DURING February 1965 we observed some absorption lines in the spectra of several stars in orthogonal planes of polarization. The… 
1962
1962
The luminous band around the horizon noted by J. Glenn in the first U.S. manned orbital flight is attributable to airglow. Dip-of…