Discovery of a Substellar Companion to the K2 III Giant ι Draconis

By S. Frink, D. Mitchell, A. Quirrenbach. 2002

147 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/a51deb4f519265080a61ca34c8936c1cddefe3cb

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

Citations in the corpus

Planets around evolved intermediate-mass stars - I. Two substellar companions in the open clusters NGC 2423 and NGC 4349 (2007, background): “Precise RV measurements have already been reported for many red giants in the solar neighbourhood, and a few planet candidates have been discovered around such stars (Frink et al. 2002; Hatzes et al. 2003, 2005, 2006; Setiawan et al. 2003, 2005; Sato et al. 2003).”
RETIRED A STARS AND THEIR COMPANIONS. III. COMPARING THE MASS–PERIOD DISTRIBUTIONS OF PLANETS AROUND A-TYPE STARS AND SUN-LIKE STARS (2009, background): “As a consequence, nearly all radial velocity surveys of IM stars are targeting evolved G- or K-type subgiants and giants (Frink et al. 2002, Setiawan et al. 2003a, Sato et al. 2005b; Johnson et al. 2006, Niedzielski et al. 2007, Döllinger et al. 2007, Lovis & Mayor 2007, Liu et al. 2009), although…”
A Planetary Companion to the Hyades Giant ϵ Tauri (2007, background): “…past few years, targets of Doppler planet searches have included not only solar-type dwarfs but also various types of stars, such as evolved (sub)giants (Frink et al. 2002; Setiawan et al. 2005; Sato et al. 2005; Hatzes et al. 2005; Johnson et al. 2006) and early-type dwarfs (Galland et al. 2005).”
Retired A Stars and Their Companions: Exoplanets Orbiting Three Intermediate-Mass Subgiants (2007, background): “Several Doppler surveys have focused on evolved, intermediate–mass stars on the red giant branch (Frink et al. 2002; Mitchell 2004; Hatzes et al. 2005; Lovis et al. 2005) and clump giant branch (Sato et al. 2003; Setiawan et al. 2003).”
THE ORBITAL EVOLUTION OF GAS GIANT PLANETS AROUND GIANT STARS (2009, background): “…has now changed, as surveys have been extended to searches for planets around more-massive stars in an evolved stage (Döllinger et al. 2007, 2009; Frink et al. 2002; Hatzes et al. 2003, 2005, 2006; Johnson et al. 2007a, 2007b, 2008; Liu et al. 2007; Lovis & Mayor 2007; Niedzielski et al. 2007,…”
Precise Radial Velocities of Giant Stars VII. Occurrence Rate of Giant Extrasolar Planets as a Function of Mass and Metallicity (2014, methodology): “In Section 2 we describe the Doppler survey at Lick Observatory.”
Precise radial velocities of giant stars. III. Spectroscopic stellar parameters (2007, background): “From the initial sample of 180 stars, companions have been announced forι Draconis (Frink et al. 2002) and Pollux (Reffert et al. 2006).”
Planet Formation around Stars of Various Masses: The Snow Line and the Frequency of Giant Planets (2007, background): “In addition, radial velocity surveys now extend over a wider range of stellar masses (e.g. Frink et al. 2002; Butler et al. 2006; Johnson et al. 2007a,b).”