Near-infrared integral-field spectra of the planet/brown dwarf companion AB Pictoris b
Context. We have already imaged a co-moving companion at a projected separation of ~260 AU from the young star AB Pic A. Evolutionary model predictions based on JHK photometry of AB Pic b suggest a mass of ~13-14 MJup, placing the object at the deuterium-
| Authors: | , |
|---|---|
| Format: | article |
| Status: | Published version |
| Publication Date: | 2010 |
| Country: | Chile |
| Language: | English |
| OAI Identifier: | oai:repositorio.anid.cl:10533/240812 |
| Online Access: | https://hdl.handle.net/10533/240812 |
| Access Level: | Open access |
| Summary: | Context. We have already imaged a co-moving companion at a projected separation of ~260 AU from the young star AB Pic A. Evolutionary model predictions based on JHK photometry of AB Pic b suggest a mass of ~13-14 MJup, placing the object at the deuterium- |
|---|