Near-IR coronagraphic imaging of the companion to HR 7672
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20031216/pdf
Reference31 articles.
1. Evolutionary models for low-mass stars and brown dwarfs: Uncertainties and limits at very young ages
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3. A low-temperature companion to a white dwarf star
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1. The Initial Mass Function Based on the Full-sky 20 pc Census of ∼3600 Stars and Brown Dwarfs;The Astrophysical Journal Supplement Series;2024-04-01
2. Detecting Exomoons from Radial Velocity Measurements of Self-luminous Planets: Application to Observations of HR 7672 B and Future Prospects;The Astronomical Journal;2023-02-20
3. Using old and new approaches: determining physical properties of brown dwarfs with empirical relations and machine learning models;Monthly Notices of the Royal Astronomical Society;2022-03-29
4. Retrieving the C and O Abundances of HR 7672 AB: A Solar-type Primary Star with a Benchmark Brown Dwarf;The Astronomical Journal;2022-03-25
5. A survey of the linear polarization of directly imaged exoplanets and brown dwarf companions with SPHERE-IRDIS;Astronomy & Astrophysics;2021-03
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