Davis, Chris J., Cervantes, B., Nisini, Brunella, Giannini, Teresa, Takami, Michihiro, Whelan, Emma Teresa, Smith, Michael D., Ray, Thomas P., Chrysostomou, Antonio C., Pyo, Tae-Soo and others. (2011) VLT integral field spectroscopy of embedded protostars: Using near-infrared emission lines as tracers of accretion and outflow. Astronomy & Astrophysics, 528 . p. 15897. ISSN 0004-6361. (doi:10.1051/0004-6361/201015897) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50085)
The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
Official URL: http://www.dx.doi.org/10.1051/0004-6361/201015897 |
Abstract
Aims. We present near-infrared spectroscopy of the forbidden emission line (FEL) and molecular hydrogen emission line (MHEL) regions at the bases of Herbig-Haro (HH) jets from seven embedded protostars: SVS 13 (the HH 7-11 progenitor), HH 26-IRS, HH 34-IRS, HH 72-IRS, HH 83-IRS, HH 300-IRS (IRAS 04239+2436) and HH 999-IRS (IRAS 06047-1117)
Methods. The integral field spectrograph, SINFONI, on the European Southern Observatory’s Very Large Telescope (VLT) was used to characterise jet parameters in these formative regions, where the jets are collimated and accelerated.
Item Type: | Article |
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DOI/Identification number: | 10.1051/0004-6361/201015897 |
Uncontrolled keywords: | shock waves ; stars ; formation ; protostars ; Herbig-Haro objects ; ISM ; jets and outflows ; mass-loss |
Subjects: | Q Science > QB Astronomy > QB460 Astrophysics |
Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
Depositing User: | Giles Tarver |
Date Deposited: | 10 Aug 2015 15:50 UTC |
Last Modified: | 05 Nov 2024 10:35 UTC |
Resource URI: | https://kar.kent.ac.uk/id/eprint/50085 (The current URI for this page, for reference purposes) |
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