Discovery of a brown dwarf companion to the star HIP 64892
We report the discovery of a bright, brown dwarf companion to the star HIP 64892, imaged with VLT/SPHERE during the SHINE exoplanet survey. The host is a B9.5V member of the Lower-Centaurus-Crux subgroup of the Scorpius Centaurus OB association. The measured angular separation of the companion (1.27...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2018-07, Vol.615, p.A160 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | We report the discovery of a bright, brown dwarf companion to the star HIP 64892, imaged with VLT/SPHERE during the SHINE exoplanet survey. The host is a B9.5V member of the Lower-Centaurus-Crux subgroup of the Scorpius Centaurus OB association. The measured angular separation of the companion (1.2705 ± 0.0023”) corresponds to a projected distance of 159 ± 12 AU. We observed the target with the dual-band imaging and long-slit spectroscopy modes of the IRDIS imager to obtain its spectral energy distribution (SED) and astrometry. In addition, we reprocessed archival NACO L-band data, from which we also recover the companion. Its SED is consistent with a young ( |
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ISSN: | 0004-6361 1432-0746 1432-0746 1432-0756 |
DOI: | 10.1051/0004-6361/201832650 |