Gee, G., Griffin, Matthew John ![]() ![]() |
Official URL: http://mnras.oxfordjournals.org/content/215/1/15P
Abstract
The authors have made submillimetre observations of the Bok globule B335 and partially resolved the cold, compact, far-infrared source detected by Keene et al. The luminosity of this source suggests that it is an embedded, low-mass, pre-main-sequence or protostellar object. From the measured size of the central source the authors conclude that it is an envelope of material accreting on to a central core and being heated by radiation from the accretion shock. Some of the energy released at the shock causes mass loss which is channelled by the surrounding envelope into a bipolar outflow. The presence of both infall and outflow in B335 indicates that it belongs to a new class of astronomical object.
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Schools > Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | Wiley-Blackwell |
ISSN: | 0035-8711 |
Last Modified: | 28 Oct 2022 09:52 |
URI: | https://orca.cardiff.ac.uk/id/eprint/75956 |
Actions (repository staff only)
![]() |
Edit Item |