scholarly journals Radial Velocity Studies of Southern Close Binary Stars. II. Spring/Summer Systems

2006 ◽  
Vol 133 (1) ◽  
pp. 169-176 ◽  
Author(s):  
Hilmar W. Duerbeck ◽  
Slavek M. Rucinski
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

Radial Velocity Studies of Close Binary Stars. II.

1999 ◽  
Vol 118 (5) ◽  
pp. 2451-2459 ◽  
Author(s):  
Slavek M. Rucinski ◽  
Wenxian Lu
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals Radial Velocity Studies of Close Binary Stars. XII.

2007 ◽  
Vol 133 (5) ◽  
pp. 1977-1987 ◽  
Author(s):  
Theodor Pribulla ◽  
Slavek M. Rucinski ◽  
George Conidis ◽  
Heide DeBond ◽  
J. R. Thomson ◽  
...  
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals Radial Velocity Studies of Close Binary Stars. IV.

2001 ◽  
Vol 122 (1) ◽  
pp. 402-412 ◽  
Author(s):  
Wenxian Lu ◽  
Slavek M. Rucinski ◽  
Waldemar OgŁłoza
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. XIII

2008 ◽  
Vol 136 (2) ◽  
pp. 586-593 ◽  
Author(s):  
Slavek M. Rucinski ◽  
Theodor Pribulla ◽  
Stefan W. Mochnacki ◽  
Evgenij Liokumovich ◽  
Wenxian Lu ◽  
...  
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

Radial Velocity Studies of Close Binary Stars. I.

1999 ◽  
Vol 118 (1) ◽  
pp. 515-526 ◽  
Author(s):  
Wenxian Lu ◽  
Slavek M. Rucinski
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals Radial Velocity Studies of Close Binary Stars. IX.

2004 ◽  
Vol 127 (3) ◽  
pp. 1712-1719 ◽  
Author(s):  
Wojtek Pych ◽  
Slavek M. Rucinski ◽  
Heide DeBond ◽  
J. R. Thomson ◽  
Christopher C. Capobianco ◽  
...  
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. XIV

2009 ◽  
Vol 137 (3) ◽  
pp. 3646-3654 ◽  
Author(s):  
Theodor Pribulla ◽  
Slavek M. Rucinski ◽  
Heide DeBond ◽  
Archie de Ridder ◽  
Toomas Karmo ◽  
...  
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals RADIAL VELOCITY STUDIES OF CLOSE BINARY STARS. XV

2009 ◽  
Vol 137 (3) ◽  
pp. 3655-3667 ◽  
Author(s):  
Theodor Pribulla ◽  
Slavek M. Rucinski ◽  
R. M. Blake ◽  
Wenxian Lu ◽  
J. R. Thomson ◽  
...  
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals Radial Velocity Studies of Close Binary Stars. III

2000 ◽  
Vol 120 (2) ◽  
pp. 1133-1139 ◽  
Author(s):  
Slavek M. Rucinski ◽  
Wenxian Lu ◽  
Stefan W. Mochnacki
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
Close Binary ◽  
Close Binary Stars

scholarly journals AM Herculis Type Stars - Magnetic Binaries

1977 ◽  
Vol 42 ◽  
pp. 238-241 ◽  
Author(s):  
W. Krzemiński
Keyword(s):  
Radial Velocity ◽  
Binary Stars ◽  
The Other ◽  
Close Binary ◽  
Polarization Spectrum ◽  
X Ray ◽  
New Class ◽  
Close Binary Stars

A new class of close binary stars, proposed to be called polars, has been discovered during recent year; its prototype is AM Her. The three known polars, AM Her, AN UMa, and W Pup, are polarization, spectrum, radial velocity, optical, and infrared variables of short periods of 3.1, 1.9, and 1.7 hours, respectively (Tapia 1977 a, b, c; Michalsky et al. 1977; Krzemiński and Serkowski 1977; Stockman et al. 1978; Herbig 1960; Cowley and Crampton 1977; Priedhorsky 1977; Greenstein et al. 1977; Berg and Duthie 1977; Szkody and Brownlee 1977; Olson 1977; Mumford 1977; Priedhorsky and Krzemiński 1978; Neugebauer et al. 1977). AM Her itself has been found to have strong soft X-ray emission in the 0.1 - 0.4 keV band (Hearn and Richardson 1977) and a hard X-ray spectrum (about half the observed 2-60 keV energy lies above 28 keV, Swank et al. 1977) both modulated with a 3.1 hour period. No X-ray emissions from the other systems have been detected so far.

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