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

EAS Publications Series EDP Sciences

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 NL Netherlands (NL) European Southern Observatory (ESO) DE Germany (DE) Eberhard Karls Universität Tübingen DE Germany (DE) Katholieke Universiteit Leuven (KUL) / Catholic University of Leuven BE Belgium (BE) High Point University US 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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