A THERMAL INFRARED IMAGING STUDY OF VERY LOW MASS, WIDE-SEPARATION BROWN DWARF COMPANIONS TO UPPER SCORPIUS STARS: CONSTRAINING CIRCUMSTELLAR ENVIRONMENTS-Reference-Cited by-同舟云学术

A THERMAL INFRARED IMAGING STUDY OF VERY LOW MASS, WIDE-SEPARATION BROWN DWARF COMPANIONS TO UPPER SCORPIUS STARS: CONSTRAINING CIRCUMSTELLAR ENVIRONMENTS

Published:2013-03-22 Issue:1 Volume:767 Page:31
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bailey Vanessa,Hinz Philip M.,Currie Thayne,Su Kate Y. L.,Esposito Simone,Hill John M.,Hoffmann William F.,Jones Terry,Kim Jihun,Leisenring Jarron,Meyer Michael,Murray-Clay Ruth,Nelson Matthew J.,Pinna Enrico,Puglisi Alfio,Rieke George,Rodigas Timothy,Skemer Andrew,Skrutskie Michael F.,Vaitheeswaran Vidhya,Wilson John C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/767/i=1/a=31/pdf

Reference85 articles.

1. PROTOPLANETARY DISK STRUCTURES IN OPHIUCHUS

2. THE YOUNG PLANET-MASS OBJECT 2M1207b: A COOL, CLOUDY, AND METHANE-POOR ATMOSPHERE

3. Predicting the properties of binary stellar systems: the evolution of accreting protobinary systems

4. FORMATION OF GIANT PLANETS BY DISK INSTABILITY ON WIDE ORBITS AROUND PROTOSTARS WITH VARIED MASSES

Cited by 31 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Moderate-resolution K-band Spectroscopy of the Substellar Companion VHS 1256 b;The Astronomical Journal;2022-09-22

2. The nature of the radio source detected towards the exoplanet system 1RXS1609.1−210524;Monthly Notices of the Royal Astronomical Society;2022-07-22

3. Characterizing the Protolunar Disk of the Accreting Companion GQ Lupi B*;The Astronomical Journal;2021-12-01

4. A survey of the linear polarization of directly imaged exoplanets and brown dwarf companions with SPHERE-IRDIS;Astronomy & Astrophysics;2021-03

5. MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4–5 μm;Astronomy & Astrophysics;2020-11-26