SIMBAD references

2004AJ....127.2871M - Astron. J., 127, 2871-2884 (2004/May-0)

The brown dwarf desert at 75-1200 AU.

McCARTHY C. and ZUCKERMAN B.

Abstract (from CDS):

We present results of a comprehensive infrared coronagraphic search for substellar companions to nearby stars. The research consisted of (1) a 178-star survey at Steward and Lick observatories, with optical follow-up from Keck Observatory, capable of detecting companions with masses greater than 30 MJ, and semimajor axes between about 140 to 1200 AU; (2) a 102-star survey using the Keck Telescope, capable of detecting extrasolar brown dwarfs and planets typically more massive than 10 MJ, with semimajor axes between about 75 and 300 AU. Only one brown dwarf companion was detected, and no planets. The frequency of brown dwarf companions to G, K, and M stars orbiting between 75 and 300 AU is measured to be 1%±1%, the most precise measurement of this quantity to date. The frequency of massive (greater than 30 MJ) brown dwarf companions at 120-1200 AU is found to be f=0.7%±0.7%. The frequency of giant planet companions with masses between 5 and 10 MJorbiting between 75 and 300 AU is measured here for the first time to be no more than ∼3%. Together with other surveys that encompass a wide range of orbital separations, these results imply that substellar objects with masses between 12 and 75 MJform only rarely as companions to stars. Theories of star formation that could explain these data are only now beginning to emerge.

Abstract Copyright:

Journal keyword(s): Stars: Binaries: General - Stars: Low-Mass, Brown Dwarfs

CDS comments: Table 2 : star PS 176 = [PS78] 176. Table 3 : * with AP and FL names not identified.

Simbad objects: 198

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2004AJ....127.2871M and select 'bookmark this link' or equivalent in the popup menu


2019.10.16-07:42:57

© Université de Strasbourg/CNRS

    • Contact