Orbits and System Masses of 14 Visual Double Stars with Early-Type Components

Details Orbits and System Masses of 14 Visual Double Stars with Early-Type Components Orbits and System Masses of 14 Visual Double Stars with Early-Type Components

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aj....133.1209d&link_type=abstract

The Astronomical Journal, Volume 133, Issue 4, pp. 1209-1216 (2007).

Astronomy and Astrophysics

Astronomy

10

Binaries: Visual, Stars: Fundamental Parameters: Masses

Scientific paper

This paper presents revised orbits and system masses of 14 visual double stars, in all of which at least one component is of early spectral type: WDS 00546+1911 (STT 20 AB), WDS 01040+3528 (HO 213), WDS 02039+4220 (STT 38 BC), WDS 03503+2535 (STT 65), WDS 06393+4200 (STT 150), WDS 08285-0231 (A551 AB), WDS 15088-4517 (SEE 219 AB), WDS 15416+1940 (HU 580 AB), WDS 16514+0113 (STT 315), WDS 17104-1544 (BU 1118 AB), WDS 19172-6640 (GLE 3), WDS 19411+1349 (KUI 93), WDS 22241-0450 (BU 172 AB), and WDS 23382+5514 (A1493). Star masses were calculated from Hipparcos parallax data whenever the precision was good enough (10 cases); otherwise, dynamical parallaxes were used, except in one case involving component multiplicity. Other physical and orbital properties of these stars are also discussed.

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