Asset Details
Do you wish to reserve the book?
The Class 0 source Barnard 1c
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
The Class 0 source Barnard 1c
Do you wish to request the book?
The Class 0 source Barnard 1c
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Journal Article
The Class 0 source Barnard 1c
2008
Overview
We present our most recent results from an ongoing study of the Class 0 source Barnard 1c in Perseus. This source is of particular interest because it exhibits evidence of strong alignment of grains all the way to the core's centre, which is contrary to all other low-mass protostellar cores observed to date. Our goal is to clarify the source of poor alignment in other sources by identifying the source of strong alignment in B1c. A central cavity has been identified in N sub(2)H super(+) emission; its anticorrelation with C super(18)O emission suggests that heating in the centre has released CO from grain mantles, in turn destroying N sub(2)H super(+). We present sensitivity-limited, high spatial resolution polarimetry data from the SubMillimeter Array and discuss the potential implications of these data.
We currently cannot retrieve any items related to this title. Kindly check back at a later time.