Resolved double-lined spectroscopic binaries: A neglected source of hypothesis-free parallaxes and stellar masses

By Dimitri Pourbaix. 2000

133 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/075a3b06a4382fb845e0042ae7eae5de7848dd8f

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. A. Tokovinin
2. B. Mason
3. W. Hartkopf
4. Eric Mamajek
5. S. Udry
6. M. Mayor
7. D. Gies
8. M. Meyer

In Computational Mechanics

1. A. Tokovinin
2. W. Hartkopf
3. B. Mason
4. Eric Mamajek
5. J. Helsel
6. S. Udry
7. M. Mayor
8. M. Meyer

In Instrumentation

1. A. Tokovinin
2. B. Mason
3. W. Hartkopf
4. S. Udry
5. M. Mayor
6. Frédéric Arenou
7. J. Helsel
8. Eric Mamajek

Citations in the corpus

• SPECKLE INTERFEROMETRY AND ORBITS OF “FAST” VISUAL BINARIES (2012, background): “This is a minor revision of the orbit by Pourbaix (2000) needed to reduce its large residual from our measure in 2009.”
• The Activity and Variability of the Sun and Sun-like Stars. I. Synoptic Ca II H and K Observations (2007, background): “However, HD 81809 is a binary with evolved components (e.g., Pourbaix 2000), so the system is not considered a solar analog.”
• THE PHASES DIFFERENTIAL ASTROMETRY DATA ARCHIVE. II. UPDATED BINARY STAR ORBITS AND A LONG PERIOD ECLIPSING BINARY (2010, methodology): “CORAVEL produced 31 two-component velocity measurements of HD 137107 A and B, reported first by Duquennoy et al. (1991) and revised by Pourbaix (2000).”
• THE HIGH ANGULAR RESOLUTION MULTIPLICITY OF MASSIVE STARS (2008, methodology): “(24) Recent orbital solutions (Tokovinin 1986; Pourbaix 2000) predict a separation of about 0.”
• DISCOVERY OF A FAINT COMPANION TO ALCOR USING MMT/AO 5 μm IMAGING (2009, background): “The systemic velocity of Mizar A is -6.3± 0.4 km s−1 (Pourbaix 2000) and that for B is -9.3± 0.1 km s−1 (Gutmann 1965).”
• Nearby stars of the Galactic disc and halo – IV (2008, unknown): “…tracks imply MA 0.81 M and MB 0.78 M , essentially in line with the orbital solutions given in Söderhjelm (1999), MA = 0.84±0.05 M , MB = 0.80 ± 0.05 M , Pourbaix (2000), MA = 0.80 ± 0.15 M , MB = 0.80 ± 0.14 M , Arenou et al. (2000), MA = 0.83± 0.09 M , MB = 0.79 ± 0.09 M , and Farrington et…”
• Multiplicity among solar-type stars (2018, background): “6 Combined spectroscopic and visual orbit by Berman (1932), Batten & van Dessel (1976), Batten et al. (1984), Heintz (1988), Batten & Fletcher (1991), and Pourbaix (2000).”