Skip to main content

NUMERICAL SIMULATION OF PROTOSTAR FORMATION IN MAGNETIZED MOLECULAR CLOUD CORES

Buy Article:

$60.90 plus tax (Refund Policy)

Abstract:

The two-dimensional numerical simulations of magnetized molecular cloud collapse has been done using integrated adaptive mesh in spherical coordinates. To take into account non-isothermality of late stages of collapse, we use a kind of "parametrical" approach to the radiative transfer through the cloud. Several numerical models are presented.

Keywords: Collapse; Interstellar medium; MHD; Molecular cloud cores; Numerical simulation; Star formation

Document Type: Research Article

DOI: http://dx.doi.org/10.1080/1055679021000040947

Affiliations: 1: Chelyabinsk State University, Br. Kashirinykh 129, Chelyabinsk, 454021, Russia 2: Keldysh Institute of Applied Mathematics, Miusskaya sq. 4, Moscow, 125047, Russia

Publication date: February 1, 2003

More about this publication?
tandf/gaat/2003/00000022/00000001/art00003
dcterms_title,dcterms_description,pub_keyword
6
5
20
40
5

Access Key

Free Content
Free content
New Content
New content
Open Access Content
Open access content
Subscribed Content
Subscribed content
Free Trial Content
Free trial content
Cookie Policy
X
Cookie Policy
Ingenta Connect website makes use of cookies so as to keep track of data that you have filled in. I am Happy with this Find out more