Complutense University Library

Subarcsecond images of CW-Tauri - constraints on disk size and jet formation

Gómez de Castro, Ana Inés (1993) Subarcsecond images of CW-Tauri - constraints on disk size and jet formation. Astrophysical journal, 412 (1, Part 2). pp. 43-46. ISSN 0004-637X

[img] PDF
Restricted to Repository staff only until 31 December 2020.

111kB

Official URL: http://adsabs.harvard.edu/abs/1993ApJ...412L..43G

View download statistics for this eprint

==>>> Export to other formats

Abstract

Subarcsecond spatial resolution images in the [S II] and [N II] + Halpha emission lines of the T Tauri star (TTS) CW Tau are presented. It is shown that CW Tau has a jet that extends up to 2.2'' (300 AU) from the star in the direction P.A. = 144-degrees. The jet emits strongly in [S II], and it is already collimated at 1.3'' (176 AU) from the star. The images also indicate that CW Tau is extended in the east-west direction and that the jet is slightly shifted to the east. This suggests that CW Tau may be a binary with the two components separated 0.20'' (28 AU). The observations are compared with the theoretical models proposed for the production of forbidden line emission regions (FLERs) and protostellar jets.


Item Type:Article
Uncontrolled Keywords:Young stellar objects; France-Hawaii telescope; high-resolution camera; circumstellar disks; forbidden-line; Stars, formation; stars, individual (cw-tauri, fm-tauri, v773-tauri); stars, pre-main-sequence
Subjects:Sciences > Mathematics > Astronomy
ID Code:16553
Deposited On:27 Sep 2012 08:45
Last Modified:27 Sep 2012 08:45

Repository Staff Only: item control page