Zobrazeno 1 - 6
of 6
pro vyhledávání: '"M. J. Plavec"'
Publikováno v:
Space Science Reviews. 28
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4b036d54988ebd46570936e13fb786db
https://doi.org/10.1007/bf00218812
https://doi.org/10.1007/bf00218812
Autor:
M. J. Plavec
Publikováno v:
Symposium - International Astronomical Union. 88:xiii-xiii
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5a51860d6041edae12d968f46f5d86a6
https://doi.org/10.1017/s0074180900064494
https://doi.org/10.1017/s0074180900064494
Publikováno v:
The Astrophysical Journal. 256:206
IUE spectra and optical scans covering the 110-680 nm interval were obtained in a search for a source which would resolve the anomalous presence of strong Balmer emission lines in the SX Cas eclipsing binary system, which is inconsistent with the usu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f4c35744845baebc1c58da14064b5c87
https://doi.org/10.1086/159897
https://doi.org/10.1086/159897
Publikováno v:
Symposium - International Astronomical Union. 88:xiii-xiii
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::305942d389d5f2394997117b46e72d49
https://doi.org/10.1017/s0074180900064482
https://doi.org/10.1017/s0074180900064482
Autor:
M. J. Plavec
Publikováno v:
The Astrophysical Journal. 275:251
The numerous emission lines in the far-UV spectrum which have been found in the Algol-type eclipsing binary U Cephei are similar to those observed in the W Serpentis stars, although they are weaker and appear only during the primary eclipse. The line
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d371c3c834e5cb5763139a7aa5fca2b9
https://doi.org/10.1086/161530
https://doi.org/10.1086/161530
Publikováno v:
The Astrophysical Journal. 282:667
Several evolved close binaries and shell stars were observed with the IPC aboard the HEAO 2 Einstein Observatory. No eclipsing target was detected, and only two of the shell binaries were detected. It is argued that there is no substantial difference
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::18d3119a0de1310ead364cbd08182c1a
https://doi.org/10.1086/162246
https://doi.org/10.1086/162246