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Infratemporal crest of sphenoid
Known as:
Crista infratemporalis alaris majoris ossis sphenoidalis
National Institutes of Health
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Papers overview
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1999
1999
Spectroscopic binary orbits from photoelectric radial velocities Paper 147: 62 Ursae Majoris
R. Griffin
,
M. Mayor
,
S. Udry
,
J. Tomkin
1999
Corpus ID: 122197817
1996
1996
SPECTROSCOPIC ORBIT OF THE TRIPLE STAR 55 URSAE MAJORIS
J. Horn
,
J. Kubát
,
+5 authors
P. Škoda
1996
Corpus ID: 117850310
1993
1993
Spectrally resolved eclipse maps of the accretion disk in UX Ursae Majoris
R. Rutten
,
V. Dhillon
,
K. Horne
,
E. Kuulkers
,
J. Paradijs
Nature
1993
Corpus ID: 4350573
ACCRETION disks play an important role in many astrophysical environments, such as active galactic nuclei, protostellar systems…
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1993
1993
The uniqueness of photometric solutions for spotted W Ursae Majoris binaries
C. Maceroni
,
F. V. Veer
1993
Corpus ID: 118268303
The perturbations frequently affecting the W UMa binaries light curves are currently explained in terms of bright/dark spots…
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1993
1993
Long-Term Light Curve of the Cataclysmic X-Ray Source 1ES1113+432 = AR Ursae Majoris
W. Wenzel
1993
Corpus ID: 116436435
1991
1991
The range of abundances of iron, chromium, and silicon over the surfaces of the CP stars ε Ursae Majoris and θ Aurigae
J. Rice
,
W. Wehlau
1991
Corpus ID: 120525442
1990
1990
Distribution of elements in rings on the surfaces of ε Ursae Majoris and θ Aurigae
J. Rice
,
W. Wehlau
1990
Corpus ID: 125713024
Les distributions des largeurs equivalentes des raies d'absoption Fe, Cr et Si a la surface des etoiles chimiquement…
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1985
1985
The Lyman alpha emission in W Ursae Majoris.
S. Rucinski
,
O. Vilhu
,
J. Whelan
1985
Corpus ID: 117119385
Resultats de la reduction de six spectres IUE-SWP a faible resolution durant une revolution orbitale de W UMa, etoile prototype…
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1980
1980
UX Ursae Majoris
A. Holm
,
R. J. Panek
,
F. H. Schiffer
1980
Corpus ID: 172931998
1974
1974
Coherent Oscillations In UX Ursae Majoris
R. Nather
,
E. L. Robinson
1974
Corpus ID: 117065045
Rapid oscillations appeared in the light curve of UX UMa and were studied from 1973 March 3 through 8, during which time they…
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