DISCOVERY OF RADIAL VELOCITY VARIABLE POST-AGB STARS FROM THE MUCHFUSS PROJECT
Reindl N, Geier S, Kupfer T, Schaffenroth V, Heber U, Barlow BN, Ostensen RH (2015)
Publication Status: Published
Publication Type: Conference contribution
Publication year: 2015
Journal
Book Volume: 71-72
Pages Range: 135-136
DOI: 10.1051/eas/1571028
Abstract
In the course of the MUCHFUSS project we have discovered five radial velocity (RV) post-AGB stars. Among them, we found the first known RV variable 0(He) star, the only second known RV variable PG 1159 close binary candidate and three RV variable, H-rich post-AGB stars of O(H)-type.
Authors with CRIS profile
Veronika Schaffenroth
Dr.Karl-Remeis-Sternwarte Bamberg, Astronomisches Institut
Ulrich Heber
Naturwissenschaftliche Fakultät
Involved external institutions
Radboud University Nijmegen
Netherlands (NL)
European Southern Observatory (ESO)
Germany (DE)
Eberhard Karls Universität Tübingen
Germany (DE)
Katholieke Universiteit Leuven (KUL) / Catholic University of Leuven
Belgium (BE)
High Point University
United States (USA) (US)
Netherlands (NL)
European Southern Observatory (ESO)
Germany (DE)
Eberhard Karls Universität Tübingen
Germany (DE)
Katholieke Universiteit Leuven (KUL) / Catholic University of Leuven
Belgium (BE)
High Point University
United States (USA) (US)
How to cite
APA:
Reindl, N., Geier, S., Kupfer, T., Schaffenroth, V., Heber, U., Barlow, B.N., & Ostensen, R.H. (2015). DISCOVERY OF RADIAL VELOCITY VARIABLE POST-AGB STARS FROM THE MUCHFUSS PROJECT. (pp. 135-136).
MLA:
Reindl, N., et al. "DISCOVERY OF RADIAL VELOCITY VARIABLE POST-AGB STARS FROM THE MUCHFUSS PROJECT." 2015. 135-136.
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