Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314

Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

16 pages, 4 figures, accepted for publication in PASJ

Scientific paper

We report the detections of two substellar companions orbiting around evolved intermediate-mass stars from precise Doppler measurements at Subaru Telescope and Okayama Astrophysical Observatory. HD 145457 is a K0 giant with a mass of 1.9 M_sun and has a planet of minimum mass m_2sini=2.9 M_J orbiting with period of P=176 d and eccentricity of e=0.11. HD 180314 is also a K0 giant with 2.6 M_sun and hosts a substellar companion of m_2sin i=22 M_J, which falls in brown-dwarf mass regime, in an orbit with P=396 d and e=0.26. HD 145457 b is one of the innermost planets and HD 180314 b is the seventh candidate of brown-dwarf-mass companion found around intermediate-mass evolved stars.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Substellar Companions to Evolved Intermediate-Mass Stars: HD 145457 and HD 180314 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-298124

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.