Cross-correlation characteristics of OB stars from IUE spectroscopy
We present a catalogue of homogeneous measures of the linewidth parameter, ve sin i, for
373 O-type stars and early B supergiants (including the separate components of 25 binary …
373 O-type stars and early B supergiants (including the separate components of 25 binary …
The Struve-Sahade effect in the optical spectra of O-type binaries-I. Main-sequence systems
N Linder, G Rauw, H Sana, M De Becker… - Astronomy & …, 2007 - aanda.org
Aims. We present a spectroscopic analysis of four massive binary systems that are known or
are good candidates to display the Struve-Sahade effect (defined as the apparent …
are good candidates to display the Struve-Sahade effect (defined as the apparent …
Evolutionary states of the two shortest period O-type overcontact binaries V382 Cyg and TU Mus
SB Qian, JZ Yuan, L Liu, JJ He… - Monthly Notices of the …, 2007 - academic.oup.com
Up to now, V382 Cyg and TU Mus are the only two discovered O-type overcontact binary
stars with periods less than two days (P= 1.8855 and 1.3873 d). Both systems contain a …
stars with periods less than two days (P= 1.8855 and 1.3873 d). Both systems contain a …
Constraining the overcontact phase in massive binary evolution-II. Period stability of known O+ O overcontact systems
Context. Given that mergers are often invoked to explain many exotic phenomena in
massive star evolution, understanding the evolutionary phase directly preceding a merger …
massive star evolution, understanding the evolutionary phase directly preceding a merger …
[HTML][HTML] Three massive binaries and the Struve-Sahade effect
DJ Stickland - The Observatory, vol. 117, p. 37-50 (1997), 1997 - adsabs.harvard.edu
Three massive binaries and the Struve-Sahade effect ADS Classic is now deprecated. It will
be completely retired in October 2019. This page will automatically redirect to the new ADS …
be completely retired in October 2019. This page will automatically redirect to the new ADS …
V606 Centauri: an early-type eclipsing contact binary
R Lorenz, P Mayer, H Drechsel - … , v. 345, p. 531-546 (1999), 1999 - adsabs.harvard.edu
We present a spectroscopic and photometric analysis of the early-type eclipsing binary V606
Cen. Based on new high-resolution CCD spectra the first radial velocity curve of this system …
Cen. Based on new high-resolution CCD spectra the first radial velocity curve of this system …
Tomographic Separation of Composite Spectra. XI. The Physical Properties of the Massive Close Binary HD 100213 (TU Muscae)
We present the results of a Doppler tomographic reconstruction of the UV spectra of the
double-lined, O binary HD 100213 based on observations made with the International …
double-lined, O binary HD 100213 based on observations made with the International …
Photospheric Heating in Colliding-Wind Binaries
The spectra of many massive binaries show secondary line depths that are deeper when the
secondary is approaching, a phenomenon we refer to as the Struve-Sahade effect. Such …
secondary is approaching, a phenomenon we refer to as the Struve-Sahade effect. Such …
The winds, metallicity, rotational velocities and mass loss rate of the hot, contact binary TU Muscae (HD100213)
RJ Pfeiffer - arXiv preprint arXiv:2407.19029, 2024 - arxiv.org
A model of the TU Muscae binary system has been developed by a study of 23 SWP
spectrophotometric images obtained with the IUE satellite telescope and downloaded from …
spectrophotometric images obtained with the IUE satellite telescope and downloaded from …
[HTML][HTML] Spectroscopic binary orbits from ultraviolet radial velocities. Paper 22: HD 48099
DJ Stickland - The Observatory, v. 116, p. 294-297 (1996), 1996 - adsabs.harvard.edu
Spectroscopic binary orbits from ultraviolet radial velocities. Paper 22: HD 480 ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …
now deprecated. It will be completely retired in October 2019. This page will automatically …