2007The Astrophysical JournalOpen access

Southern Very Low Mass Stars and Brown Dwarfs in Wide Binary and Multiple Systems

J. A. Caballero

Open full text 60 citations

Abstract

The results of the Königstuhl survey in the Southern Hemisphere are presented. I have searched for common proper motion companions to 173 field very low mass stars and brown dwarfs with spectral types >M5.0 V and magnitudes J ≲ 14.5 mag. I have measured for the first time the common proper motion of two new wide systems containing very low mass components, Königstuhl 2 AB and 3 A-BC. Together with Königstuhl 1 AB and 2M 0126-50 AB, they are among the widest systems in their respective classes ( r = 450-11,900 AU). I have determined the minimum frequency of field wide multiples ( r > 100 AU) with late-type components at 5.0% ± 1.8% and the frequency of field wide late-type binaries with mass ratios q > 0.5 at 1.2% ± 0.9%. These values represent a key diagnostic of evolution history and low-mass star and brown dwarf formation scenarios. In addition, the proper motions of 62 field very low mass dwarfs are measured here for the first time.

Open-access reader

About this research paper

What this paper is about

The results of the Königstuhl survey in the Southern Hemisphere are presented. I have searched for common proper motion companions to 173 field very low mass stars and brown dwarfs with spectral types >M5.0 V and magnitudes J ≲ 14.5 mag. I have measured for the first time the common proper motion of two new wide systems containing very low mass components, Königstuhl 2 AB and 3 A-BC. Together with Königstuhl 1 AB and 2M 0126-50 AB, they are among the widest systems in their respective classes ( r = 450-11,900 AU). I have determined the minimum frequency of field wide multiples ( r > 100 AU) with late-type components at 5.0% ± 1.8% and the frequency of field wide late-type binaries with mass ratios q > 0.5 at 1.2% ± 0.9%. These values represent a key diagnostic of evolution history and low-mass star and brown dwarf formation scenarios. In addition, the proper motions of 62 field very low mass dwarfs are measured here for the first time.

Why it matters

OpenAlex reports 60 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

The results of the Königstuhl survey in the Southern Hemisphere are presented. I have searched for common proper motion companions to 173 field very low mass stars and brown dwarfs with spectral types >M5.0 V and magnitudes J ≲ 14.5 mag. I have measured for the first time the common proper motion of two new wide systems containing very low mass components, Königstuhl 2 AB and 3 A-BC. Together with Königstuhl 1 AB and 2M 0126-50 AB, they are among the widest systems in their respective classes ( r = 450-11,900 AU). I have determined the minimum frequency of field wide multiples ( r > 100 AU) with late-type components at 5.0% ± 1.8% and the frequency of field wide late-type binaries with mass ratios q > 0.5 at 1.2% ± 0.9%. These values represent a key diagnostic of evolution history and low-mass star and brown dwarf formation scenarios. In addition, the proper motions of 62 field very low mass dwarfs are measured here for the first time.

Key concepts: Brown dwarf, Physics, Astrophysics, Proper motion, Low Mass, Stars, Stellar classification, Field (mathematics)

Related papers

Back to paper searchBrowse research topicsOriginal source
Southern Very Low Mass Stars and Brown Dwarfs in Wide Binary and Multiple Systems — Research Paper | ScholarLens