Results 41 to 50 of about 2,099,705 (77)
X-ray observations of AM Herculis from OSO-8 [PDF]
The white dwarf binary system AM Herculis (2A1815+500) was observed in X-rays at both low energies (E less 10 keV) and higher energies. The exact shape of the spectrum, particularly at the higher energies, has yet to be determined.
Frost, K. J. +5 more
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Indirekte Abbildungsverfahren angewandt auf AM Herculis-Sterne
AM Herculis-Sterne sind enge Doppelsterne, die aus einem weißen Zwerg mit starkem Magnetfeld und einem Hauptreihenstern bestehen. Letzterer verliert Materie an den weißen Zwerg, wobei das Magnetfeld die Materie zu den Magnetpolen leitet, wo die ...
Staude, Andreas
core +1 more source
Kepler observations of Am stars [PDF]
We present an analysis of high-resolution spectra for two pulsating Am stars in the Kepler field. The stellar parameters derived in this way are important because parameters derived from narrow-band photometry may be affected by the strong metal lines in
Eyer, L. +16 more
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Laboratory analogue of a supersonic accretion column in a binary star system. [PDF]
Cross JE +24 more
europepmc +1 more source
Formation of high-field magnetic white dwarfs from common envelopes. [PDF]
Nordhaus J +4 more
europepmc +1 more source
Herculis Ciofani Sulmonensis in P. Ovidii Nasonis : Libros de Ponto : Observationes
Con: Antiquiss a Nobiliss urbis sulmonis descriptio... con port e pax. propias -- Con: Herculis Ciofani Sulmoniensis in P. Ovisçdii Nasonis Halieuticon... con port. e pax. propias -- Con: Herculis Ciofani Sulmoniensis in P.
Ex offiina Christophoti Plantini +2 more
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Spectroscopic survey of Kepler stars – II. FIES/NOT observations of A- and F-type stars
We have analysed high-resolution spectra of 28 A and 22 F stars in the Kepler field, observed using the Fibre-Fed Échelle Spectrograph at the Nordic Optical Telescope. We provide spectral types, atmospheric parameters and chemical abundances for 50 stars.
S. J. Murphy +21 more
core +1 more source
On the Material Ejected from Novae. [PDF]
Payne-Gaposchkin C, Gaposchkin S.
europepmc +1 more source
Accretion and magnetic field structure in AM Herculis systems
Detailed spectroscopic studies of the magnetic white dwarfs in the AM Herculis type systems have shown that in most systems the magnetic white dwarf has two dominant poles with field strengths that differ by a factor ~1.5-2 indicating non dipolar field ...
Wickramasinghe, Dayal, Ferrario, Lilia
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Notes on Binary Stars: V. The Determination by Least-Squares of the Elements of Spectroscopic Binaries. [PDF]
Sterne TE.
europepmc +1 more source

