SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC) IX: THE PLANETARY-MASS DOMAIN OF CHAMAELEON-I AND UPDATED MASS FUNCTION IN LUPUS-3
Authors:
- 10 September 2015
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 810 (2) , 159
Abstract
No abstract availableAll Related Versions
This publication has 74 references indexed in Scilit:
- A NEAR-INFRARED SPECTROSCOPIC STUDY OF YOUNG FIELD ULTRACOOL DWARFSThe Astrophysical Journal, 2013
- Spectroscopy of brown dwarf candidates in IC 348 and the determination of its substellar IMF down to planetary massesAstronomy & Astrophysics, 2013
- A HYBRID SCENARIO FOR THE FORMATION OF BROWN DWARFS AND VERY LOW MASS STARSThe Astrophysical Journal, 2012
- Spectroscopy of new brown dwarf members ofρ Ophiuchi and an updated initial mass functionAstronomy & Astrophysics, 2012
- Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formationMonthly Notices of the Royal Astronomical Society, 2011
- THE YOUNG PLANET-MASS OBJECT 2M1207b: A COOL, CLOUDY, AND METHANE-POOR ATMOSPHEREThe Astrophysical Journal Letters, 2011
- CLOUDS AND CHEMISTRY IN THE ATMOSPHERE OF EXTRASOLAR PLANET HR8799bThe Astrophysical Journal, 2011
- EPISODIC ACCRETION AT EARLY STAGES OF EVOLUTION OF LOW-MASS STARS AND BROWN DWARFS: A SOLUTION FOR THE OBSERVED LUMINOSITY SPREAD IN H-R DIAGRAMS?The Astrophysical Journal, 2009
- Stellar, brown dwarf and multiple star properties from hydrodynamical simulations of star cluster formationMonthly Notices of the Royal Astronomical Society, 2008
- Characterizing Young Brown Dwarfs Using Low‐Resolution Near‐Infrared SpectraThe Astrophysical Journal, 2007