Towards a consistent model of the hot quadruple system HD 93206=QZ Carin ae II. N-body model

Broz M, Harmanec P, Zasche P, Catalan-Hurtado R, Barlow BN, Frondorf W, Wolf M, Drechsel H, Chini R, Nasseri A, Labadie-Bartz J, Christie GW, Walker WSG, Blackford M, Blane D, Henden AA, Bohlsen T, Bozic H, Jonak J (2022)

Publication Type: Journal article

Publication year: 2022

Journal

Astronomy & Astrophysics EDP Sciences

Book Volume: 666

DOI: 10.1051/0004-6361/202243596

Abstract

Aims. HD 93206 is a massive early-type stellar system composed of components resolved by direct imaging (Ab, Ad, B, C, D) and a compact subsystem (Aa1, Aa2, Ac1, Ac2). Its geometry was already determined on the basis of extensive photometric, spectroscopic, and interferometric observations. However, the fundamental absolute parameters are still not known precisely enough.

Authors with CRIS profile

Horst Drechsel Dr.Karl-Remeis-Sternwarte Bamberg, Astronomisches Institut

Involved external institutions

University of São Paulo / Universidade de São Paulo (USP)

Brazil (BR) University of Zagreb / Sveučilište u Zagrebu

Croatia (HR) Univerzita Karlova v Praze / Charles University in Prague

Czech Republic (CZ) High Point University

United States (USA) (US) American Association of Variable Star Observers (AAVSO)

United States (USA) (US) Variable Stars South (VSS)

New Zealand (NZ) Astronomical Society of Southern Africa (ASSA)

South Africa (ZA) Ruhr-Universität Bochum (RUB)

Germany (DE)

How to cite

APA:

Broz, M., Harmanec, P., Zasche, P., Catalan-Hurtado, R., Barlow, B.N., Frondorf, W.,... Jonak, J. (2022). Towards a consistent model of the hot quadruple system HD 93206=QZ Carin ae II. N-body model. Astronomy & Astrophysics, 666. https://doi.org/10.1051/0004-6361/202243596

MLA:

Broz, M., et al. "Towards a consistent model of the hot quadruple system HD 93206=QZ Carin ae II. N-body model." Astronomy & Astrophysics 666 (2022).

BibTeX: Download