Projects per year
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 language | English |
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Pages (from-to) | 1658-1664 |
Number of pages | 7 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 379 |
DOIs | |
Publication status | Published - 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
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Dive into the research topics of 'Molecular hydrogen emission from discs in the eta Chamaeleontis cluster'. Together they form a unique fingerprint.Projects
- 2 Finished
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Astrophysics at St Andrews: Astrophysics at St.Andrews
Cameron, A. C. (PI) & Horne, K. D. (CoI)
1/04/06 → 31/03/11
Project: Standard
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Research Fellowship - PP/C001524/1: How common is the Earth?
Greaves, J. S. (PI)
1/10/05 → 30/09/10
Project: Fellowship