Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.336.1099a&link_type=abstract
Monthly Notice of the Royal Astronomical Society, Volume 336, Issue 4, pp. 1099-1108.
Astronomy and Astrophysics
Astronomy
10
Binaries: General, Stars: Early-Type, Stars: Fundamental Parameters, Stars: Individual: Cpd: 59°2636, Open Clusters And Associations: Individual: Trumpler 16, X-Rays: Stars
Scientific paper
High-resolution optical spectroscopy of CPD - 59°2636, one of the O-type stars in the open cluster Trumpler 16 in the Carina Nebula, reveals this object to be a multiple system displaying triple lines which we label as components A, B and C of spectral types O7 V, O8 V and O9 V, respectively. From our radial velocity measurements we find that the components A and B form a close binary with a period of 3.6284 d, and we obtain the first circular radial velocity orbit for this system with semi-amplitudes of 184 and 192 km s-1, leading to minimum masses of 10.1 and 9.7 Msolar. We find that the component C is a single lined binary with a period of 5.034 d and semi-amplitude of 48 km s-1. We also analyse the X-ray radiation from CPD - 59°2636, finding neither appreciable overluminosity nor phase-related X-ray flux variations.
Albacete Colombo Juan Facundo
Corcoran Michael F.
Morrell Nidia I.
Niemela Virpi S.
Rauw Gregor
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