Molecular hydrogen emission from discs in the eta Chamaeleontis cluster

S. K. Ramsay Howat, J. S. Greaves

Research output: Contribution to journalArticlepeer-review

23 Citations (Scopus)

Abstract

Discs in the 6 Myr old cluster eta Chamaeleontis were searched for emission from hot H-2. Around the M3 star ECHA J0843.3-7905, we detect circumstellar gas orbiting at similar to 2 au. If the gas is ultraviolet excited, the ro-vibrational line traces a hot gas layer supported by a disc of mass similar to 0.03M(circle dot), similar to the minimum mass solar nebula. Such a gas reservoir at 6 Myr would promote the formation and the inwards migration of gas giant planets.

Original languageEnglish
Pages (from-to)1658-1664
Number of pages7
JournalMonthly Notices of the Royal Astronomical Society
Volume379
DOIs
Publication statusPublished - 21 Aug 2007

Keywords

  • circumstellar matter
  • planetary systems : formation
  • infrared : stars
  • MAIN-SEQUENCE STARS
  • ROTATIONAL H-2 EMISSION
  • T-TAURI STAR
  • PROTOPLANETARY DISK
  • YOUNG STARS
  • DEBRIS DISKS
  • ACCRETION
  • EVOLUTION
  • GAS
  • SPECTROSCOPY

Fingerprint

Dive into the research topics of 'Molecular hydrogen emission from discs in the eta Chamaeleontis cluster'. Together they form a unique fingerprint.

Cite this