HUBRIG, Swetlana, Zdeněk MIKULÁŠEK, M. SCHÖLLER, J. F. GONZÁLES, O. SCHÜTZ, B. STELZER, Miloslav ZEJDA, Ladislav ŠMELCER and Luboš BRÁT. A Study of the Herbig Be Binary/FU Orionis Object Z CMa. In A. Prša, M. Zejda. ASP Conference Series 435 - Binaries - Key to Comprehension to the Universe. San Francisco, USA: Astronomical Society of the Pacific, 2010, p. 343-344. ISBN 978-1-58381-750-6.
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Basic information
Original name A Study of the Herbig Be Binary/FU Orionis Object Z CMa
Name in Czech Studium Herbigovské Be dvojhvězdy/FU Ori objektu Z CMa
Authors HUBRIG, Swetlana (276 Germany), Zdeněk MIKULÁŠEK (203 Czech Republic, guarantor, belonging to the institution), M. SCHÖLLER (276 Germany), J. F. GONZÁLES (32 Argentina), O. SCHÜTZ (276 Germany), B. STELZER (380 Italy), Miloslav ZEJDA (203 Czech Republic, belonging to the institution), Ladislav ŠMELCER (203 Czech Republic) and Luboš BRÁT (203 Czech Republic, belonging to the institution).
Edition San Francisco, USA, ASP Conference Series 435 - Binaries - Key to Comprehension to the Universe, p. 343-344, 2 pp. 2010.
Publisher Astronomical Society of the Pacific
Other information
Original language English
Type of outcome Proceedings paper
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
RIV identification code RIV/00216224:14310/10:00049410
Organization unit Faculty of Science
ISBN 978-1-58381-750-6
UT WoS 000289880000083
Keywords (in Czech) FU Ori; Herbig; Be dvojhvězdy; Z CMa
Keywords in English FU Ori; Herbig; Be binaries; Z CMa
Tags AKb, rivok
Tags International impact
Changed by Changed by: doc. RNDr. Miloslav Zejda, Ph.D., učo 169695. Changed: 28/1/2013 10:07.
Abstract
ZCMa is a young visual binary star with a FU Ori companion. The primary star is in an outburst state since February 2008. We acquired photometric, spectroscopic, spectropolarimetric, and X-ray Chandra observations to study the mechanism causing violent outbursts in this kind of systems.
Abstract (in Czech)
ZCMa je mladá vizuální dvojhvězda se složkou typu FU Ori. Primární složka je ve stádiu zjasnění od února 2008. Získali jsme fotometrická, spektroskopická, spektropolarimetrická a rtg. pozorování z družice Chandra ke studiu mechanismu způsobujícího prudké zjasnění v tomto typu soustav.
Links
GD205/08/H005, research and development projectName: Fyzika Slunce, hvězd a hvězdných soustav
Investor: Czech Science Foundation, Physics of Sun, stars, and stellar systems
IAA301630901, research and development projectName: Rozložení energie ve spektru horkých hvězd a jeho proměnnost
Investor: Academy of Sciences of the Czech Republic, Spectral energy distribution of hot stars and its variability
PrintDisplayed: 28/4/2024 19:24