ROTATIONAL AND RADIAL VELOCITIES FOR A SAMPLE OF 761 HIPPARCOS GIANTS AND THE ROLE OF BINARITY
By Alessandro Massarotti, D. Latham, R. Stefanik, J. Fogel. 2007
366 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Computational Mechanics
View Paper: https://www.semanticscholar.org/paper/6b92115653463396726e8e61472a4fde47a8798d
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In Astronomy and Astrophysics
- J. Johnson
- G. Marcy
- B. Bowler
- Debra A. Fischer
- G. Henry
- Timothy Morton
- Michael C. Liu
- Andrew W. Howard
In Computational Mechanics
Citations in the corpus
- AN AMR STUDY OF THE COMMON-ENVELOPE PHASE OF BINARY EVOLUTION (2011, background): “This corresponds to an initial surface velocity for the red giant of about 35 km s−1, which is within the observed range for red giants in short-period binaries (Massarotti et al. 2008).”
- SPECTROSCOPIC ORBITS FOR 15 LATE-TYPE STARS (2016, background): “For example, while our period of 894 days agrees with the period of 898.1 days found by Massarotti et al. (2008), our eccentricity is about 25% smaller.”
- Stellar Parameters and Elemental Abundances of Late-G Giants (2008, methodology): “…ve sini values with the literature values: filled circles are those from de Medeiros and Mayor (1999) (128 stars in common), while open triangles are those from Massarotti et al. (2008) (plotted for 96 stars out of 157 stars in common, where 61 stars with ve sin iMassarotti = 0 are excluded).”
- RETIRED A STARS AND THEIR COMPANIONS. III. COMPARING THE MASS–PERIOD DISTRIBUTIONS OF PLANETS AROUND A-TYPE STARS AND SUN-LIKE STARS (2009, background): “…binaries and include HD 8375 (discussed in §3.1), HD 65938 (Pourbaix et al. 2004; Massarotti et al. 2008), HD 179799 (Setiawan et al. 2003b; Setiawan et al. 2004; Massarotti et al. 2008), and HD 210211 (spectroscopic triple system; Horch et al. 2002; Pourbaix et al. 2004; Massarotti et al. 2008).”
- XHIP: An extended hipparcos compilation (2011, background): “Our “B”-grade sources, in order of preference are: Lopez-Santiago et al., 2010; Massarotti et al., 2008; Guillout et al., 2009; Soubiran et al., 2003; Holmberg et al., 2007; Gizis et al., 2002; White et al., 2007; Torres et al., 2006; Kharchenko et al., 2007.”