scholarly journals Very Low‐Mass Stars and Brown Dwarfs of the Young Open Cluster IC 2391

2001 ◽  
Vol 134 (1) ◽  
pp. 103-114 ◽  
Author(s):  
David Barrado y Navascues ◽  
John R. Stauffer ◽  
Cesar Briceno ◽  
Brian Patten ◽  
Nigel C. Hambly ◽  
...  
Keyword(s):  
Open Cluster ◽  
Brown Dwarfs ◽  
Low Mass Stars ◽  
Young Open Cluster ◽  
Low Mass

A Search for Brown Dwarfs in the Alpha Persei Cluster

2003 ◽  
Vol 211 ◽  
pp. 179-180
Author(s):  
Nicolas Lodieu ◽  
Mark McCaughrean ◽  
Jérôme Bouvier ◽  
David Barrado y Navascués ◽  
John R. Stauffer
Keyword(s):  
Near Infrared ◽  
Open Cluster ◽  
Brown Dwarfs ◽  
Wide Field ◽  
Brown Dwarf ◽  
Young Open Cluster ◽  
Low Mass ◽  
Alpha Persei ◽  
Calar Alto ◽  
Infrared Survey

We present preliminary results from a deep near-infrared survey of a ~ 1 square degree area in the young open cluster Alpha Persei using the wide-field Omega-Prime camera on the Calar Alto 3.5m telescope, yielding a list of new low-mass cluster members, including brown dwarf candidates.

scholarly journals Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?

2010 ◽  
Vol 510 ◽  
pp. A27 ◽  
Author(s):  
S. Boudreault ◽  
C. A. L. Bailer-Jones ◽  
B. Goldman ◽  
T. Henning ◽  
J. A. Caballero
Keyword(s):  
Open Cluster ◽  
Brown Dwarfs ◽  
Mass Function ◽  
Low Mass Stars ◽  
Low Mass ◽  
Cluster A

scholarly journals Photometry and membership for low mass stars in the young open cluster NGC 2516

2001 ◽  
Vol 375 (3) ◽  
pp. 863-889 ◽  
Author(s):  
R. D. Jeffries ◽  
M. R. Thurston ◽  
N. C. Hambly
Keyword(s):  
Open Cluster ◽  
Low Mass Stars ◽  
Young Open Cluster ◽  
Low Mass

scholarly journals Modelling Planet Formation by Capture-Theory Interactions

2004 ◽  
Vol 202 ◽  
pp. 244-246
Author(s):  
Michael M. Woolfson ◽  
Stephen Oxley
Keyword(s):  
Smoothed Particle Hydrodynamics ◽  
Planet Formation ◽  
Open Cluster ◽  
Brown Dwarfs ◽  
Low Mass Stars ◽  
Capture Theory ◽  
Particle Hydrodynamics ◽  
Smoothed Particle ◽  
Solar Type ◽  
Low Mass

Diffuse low-mass stars and brown dwarfs coexist with condensed solar-type stars in the embedded stage of a developing open cluster. It is shown by smoothed-particle-hydrodynamics modelling that interactions between stars and protostars leads to disruption of the protostar to form protoplanets that can then be captured by the star.

scholarly journals Primeval very low-mass stars and brown dwarfs – II. The most metal-poor substellar object

2017 ◽  
Vol 468 (1) ◽  
pp. 261-271 ◽  
Author(s):  
Z. H. Zhang 张曾华 ◽  
D. Homeier ◽  
D. J. Pinfield ◽  
N. Lodieu ◽  
H. R. A. Jones ◽  
...  
Keyword(s):  
Brown Dwarfs ◽  
Low Mass Stars ◽  
Low Mass
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