# Giant planets around two intermediate-mass evolved stars and confirmation of the planetary nature of HIP 67851c

@article{Jones2015GiantPA,
title={Giant planets around two intermediate-mass evolved stars and confirmation of the planetary nature of HIP 67851c},
author={M. I. Jones and James S. Jenkins and Patricio M. Rojo and Claudio Melo},
journal={Astronomy and Astrophysics},
year={2015},
volume={580}
}
• Published 25 May 2015
• Physics, Geology
• Astronomy and Astrophysics
Context. Precision radial velocities are required to discover and ch aracterize planets orbiting nearby stars. Optical and near infrared spectra that exhibit many hundreds of absorption lines can allow the m s −1 precision levels required for such work. However, this means that studies have generally focused on solar-type dwarf stars. After the main-sequence, intermediate-mass star s (former AF stars) expand and rotate slower than their progenitors, th us thousands of narrow absorption lines…

## Figures and Tables from this paper

• Physics, Geology
• 2016
Context. Exoplanet searches have revealed interesting correlations between the stellar properties and the occurrence rate of planets. In particular, different independent surveys have demonstrated
• Physics, Geology
• 2017
For over 10 years, we have carried out a precise radial velocity (RV) survey to find substellar companions around evolved G,K-type stars to extend our knowledge of planet formation and evolution. We
• Physics, Geology
• 2020
As part of the search for planets around evolved stars, we can understand planet populations around significantly higher-mass stars than the Sun on the main sequence. This population is difficult to
• Physics, Geology
• 2016
Context. For over 12 yr, we have carried out a precise radial velocity (RV) survey of a sample of 373 G- and K-giant stars using the Hamilton Echelle Spectrograph at the Lick Observatory. There are,
• Physics, Geology
• 2016
We report the discovery of 24 spectroscopic binary companions to giant stars. We fully constrain the orbital solution for 6 of these systems. We cannot unambiguously derive the orbital elements for
• Physics, Geology
• 2016
We report the discovery of a substellar companion around the giant star HIP 67537. Based on precision radial velocity measurements from CHIRON and FEROS high-resolution spectroscopic data, we derived
• Physics, Geology
The Astrophysical Journal Supplement Series
• 2022
We analyze 5108 AFGKM stars with at least five high-precision radial velocity points, as well as Gaia and Hipparcos astrometric data, utilizing a novel pipeline developed in previous work. We find
• Physics, Geology
Astronomy & Astrophysics
• 2020
Aims. We are studying the influence of stellar multiplicity on exoplanet systems and, in particular, systems that have been detected via radial-velocity searches. We are specifically interested in
• Physics, Geology
Monthly Notices of the Royal Astronomical Society
• 2018
We report the direct detection of a fully convective, early-to-mid M-dwarf companion orbiting the star HD 86006, using ESO-SPHERE during Science Verification as part of the SAFARI program.
• Physics, Geology
The Astronomical Journal
• 2019
The discovery of thousands of planetary systems by Kepler has demonstrated that planets are ubiquitous. However, a major challenge has been the confirmation of Kepler planet candidates, many of which

## References

SHOWING 1-10 OF 48 REFERENCES

• Physics, Geology
• 2014
Context: More than 50 exoplanets have been found around giant stars, revealing different properties when compared to planets orbiting solar-type stars. In particular, they are Super-Jupiters and are
• Physics, Geology
• 2014
Context: So far more than 60 substellar companions have been discovered around giant stars. These systems present physical and orbital properties that contrast to those detected orbiting less evolved
• Physics, Geology
• 2014
(abridged) We have obtained precise radial velocities for a sample of 373 G and K type giants at Lick Observatory regularly over more than 12 years. Planets have been identified around 15 giant
• Physics, Geology
• 2009
We present an analysis of ∼5 years of Lick Observatory radial velocity measurements targeting a uniform sample of 31 intermediate-mass (IM) subgiants (1.5 ≲ M*/M☉≲ 2.0) with the goal of measuring the
• Physics, Geology
Science
• 2010
The planetary findings derived from the first six weeks of observations with the Kepler mission are summarized, which include the detection of five new exoplanets, which confirm the existence of planets with densities substantially lower than those predicted for gas giant planets.
• Physics, Geology
• 2013
Context. More than 40 planets have been found around giant stars, revealing a lack of systems orbiting interior to ∼0.6 AU. This observational fact contrasts with the planetary population around
• Physics, Geology
• 2011
Context. To date, more than 30 planets have been discovered around giant stars, but only one of them has been found to be orbiting within 0.6 AU from the host star, in direct contrast to what is
• Physics, Geology
• 2008
We present the results of radial velocity measurements of two samples of active stars. The first sample contains field G and K giants across the Red Giant Branch, whereas the second sample consists
• Physics, Geology
• 2014
We report the discovery of a new planetary system around the K giant $\eta$ Cet (HIP 5364, HD 6805) based on 118 high-precision optical radial velocities taken at Lick Observatory since July 2000.
• Physics, Geology
• 2005
We report on the radial-velocity variability of G-type giants based on the results of precise Doppler measurements of 57 stars that were observed for the first 3 years of the Okayama Planet Search