| Issue |
A&A
Volume 383, Number 2, FebruaryIV 2002
|
|
|---|---|---|
| Page(s) | 598 - 602 | |
| Section | The Sun | |
| DOI | https://doi.org/10.1051/0004-6361:20011605 | |
| Published online | 15 February 2002 | |
Imaging and spectroscopic studies of Haro 6-19 (HH319)*
1
Byurakan Astrophysical Observatory, Aragatsotn prov., 378433 Armenia and Isaac Newton Institute of Chile, Armenian Branch e-mail: tigmov@bao.sci.am
2
Kokugakuin University, Higashi, Shibuya-ku, Tokyo 150-8440, Japan e-mail: ogura@kokugakuin.ac.jp
3
Special Astrophysical Observatory, N.Arkhyz, Karachaevo-Cherkesia 369167, Russia e-mail: vafan@sao.ru
Corresponding author: T. Yu. Magakian, tigmag@sci.am
Received:
31
August
2001
Accepted:
24
October
2001
We performed morphological and spectro-imaging investigations of the little-studied HH object Haro 6-19 (HH319). Besides the main object, two other small HH knots were found. The images of the object in various spectral lines and maps of radial velocity and electronic density are presented. Either of the T Tauri stars FY and FZ Tau is suggested as the possible exciting source. The spatial distribution of the density and radial velocity in the object, combined with other evidence, shows that HH319 could be a shocked cloudlet. In many aspects HH319 is similar to HH29 in L1551.
Key words: ISM: individual objects: HH319 / Herbig-Haro objects / ISM: kinematics and dynamics
© ESO, 2002
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