Squamosal margin of sphenoid

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

Topic mentions per year

Topic mentions per year

1943-2008
01219432007

Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2002
2002
We present far-ultraviolet (905 – 1182 Å), time-series spectroscopy of the eclipsing, novalike cataclysmic variable, UX UMa… (More)
  • figure 1
  • figure 2
  • figure 3
  • figure 4
  • figure 5
Is this relevant?
2000
2000
We present a surface abundance Doppler image of singly–ionized calcium for the Bp star UMa based on high signal-to-noise CCD… (More)
  • figure 1
  • table 2
  • figure 2
  • figure 3
  • figure 5
Is this relevant?
1999
1999
  • HV Ursae Majoris
  • 1999
We present the first UBV and uvby photometric observations for the short period variable star HV Ursae Majoris classified as a… (More)
  • figure 1
  • figure 3
  • table 2
  • figure 4
  • table 3
Is this relevant?
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)
  • table 1
  • figure 1
  • table 2
  • table 3
  • table 4
Is this relevant?
1997
1997
Possible planetary objects have now been discovered1–9 orbiting nine different main-sequence stars. These companion objects (some… (More)
Is this relevant?
1993
1993
ACCRETION disks play an important role in many astrophysical environments, such as active galactic nuclei, protostellar systems… (More)
Is this relevant?
1984
1984
SU Ursae Majoris systems are short-period binary dwarf novae characterized by two distinct classes of outbursts: ‘normal… (More)
Is this relevant?
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)
Is this relevant?
1943
1943
  • Nature
  • 1943
 
Is this relevant?
1943
1943
  • Nature
  • 1943
 
Is this relevant?