Direct Imaging discovery of a second planet candidate around the possibly transiting planet host CVSO 30

2016/05/13 by T. O. B. Schmidt, R. Neuhäuser, C. Briceño +12 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Direct imaging #Exoplanet #Host (biology) #Planet #Planetary system #Solar System #Stellar, planetary, and galactic studies #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201526326

published as A&A 593, A75 (2016) · 15 pages, 16 figures, accepted for publication in A&A

openalex publication_date 2016/05/13 · arxiv created 2016/05/17 · openalex created_date 2016/06/24 · arxiv updated 2016/09/28 · openalex updated_date 2026/08/05

Abstract

Context. Direct imaging has developed into a very successful technique for the detection of exoplanets in wide orbits, especially around young stars. Directly imaged planets can be both followed astrometrically on their orbits and observed spectroscopically and thus provide an essential tool for our understanding of the early solar system.

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Cited by

• Evidence that the Planetary Candidate CVSO30c is a Background Star from Optical, Seeing-limited Data