Rotation and differential rotation in field F- and G-type stars

By A. Reiners, J. Schmitt. 2003

143 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/09adbc62678229ba220cdfb1f2e79773d69d9df0

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. Reiners
2. J. Donati
3. G. Basri
4. P. Petit
5. N. Piskunov
6. T. Reinhold
7. O. Kochukhov
8. V. Makaganiuk

In Instrumentation

1. A. Reiners
2. T. Reinhold
3. S. Simón-Díaz
4. G. Basri
5. A. Herrero
6. O. Kochukhov
7. N. Piskunov
8. V. Makaganiuk

Citations in the corpus

• Observations of Cool-Star Magnetic Fields (2012, methodology): “Reiners and Schmitt (2003b) used a similar approach but iteratively optimizing the weights of individual lines so that the fit to the spectrum is improved.”
• Rotation and differential rotation of active Kepler stars (2013, methodology): “Using the Fourier transform method Reiners & Schmitt (2003) also found that α increases with rotation period for F-G stars.”
• Fourier method of determining the rotational velocities in OB stars (2007, methodology): “There are numerous papers illustrating its use in determining v sin i in later type stars (Smith 1976; Gray 1980; Royer et al. 2002a,b; Reiners & Schmitt 2003); however, there is no comprehensive study applying this technique to early-type stars except the one by Ebbets (1979), who analyzed a…”
• Radial Velocity Search for Extrasolar Planets in Visual Binary Systems (2009, background): “…III 104.9 3800 27.94 1.2 (a) BDS 10966A 203857 105637 6.45 K5 III 365.4 70000 3.54 (a) de Medeiros and Mayor (1999), (b) Nordström et al. (2004), (c) Desidera et al. (2006) (d) Fekel (1997), (e) Hale (1994), (f) Gondoin (1999), (g) Reiners and Schmitt (2003), (h) Allende Prieto and Lambert (1999).”
• The spinning-top Be star Achernar from VLTI-VINCI (2003, background): “Although well studied in the literature, the effects of rotation have rarely been tested against accurate enough observations (Reiners & Schmitt 2003, van Belle et al. 2001), a gap bridged by our interferometric observations of Achernar.”
• Least-squares deconvolution of the stellar intensity and polarization spectra (2010, methodology): “A modification of the LSD method was also employed in the search for stellar differential rotation through the line profile analysis (Reiners & Schmitt 2003).”
• The dependence of differential rotation on temperature and rotation (2004, background): “We discuss the results of Reiners & Schmitt (2003) (RS03) in§3.”
• Accurate fundamental parameters for 23 bright solar-type stars (2010, result): “Our results are in general agreement with similar investigations in the literatue, identified by the first author in the Table: Saar & Osten (1997), Valenti & Fischer (2005), Reiners & Schmitt (2003), Dravinset al. (1993), and Allende Prieto et al. (2002).”