Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/200913011/pdf
Reference71 articles.
1. Structure of the Praesepe Star Cluster
2. Brown dwarf populations in open clusters
3. The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
4. The Distances to Open Clusters from Main‐Sequence Fitting. III. Improved Accuracy with Empirically Calibrated Isochrones
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2. The Factory and the Beehive. IV. A Comprehensive Study of the Rotation X-Ray Activity Relation in Praesepe and the Hyades;The Astrophysical Journal;2022-05-01
3. Goodness-of-fit test for isochrone fitting in the Gaia era;Astronomy & Astrophysics;2021-05
4. Two close binaries across the hydrogen-burning limit in the Praesepe open cluster;Monthly Notices of the Royal Astronomical Society;2020-08-21
5. Spectral library of age-benchmark low-mass stars and brown dwarfs;Monthly Notices of the Royal Astronomical Society;2019-12-27
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