Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-27T03:49:46.518Z Has data issue: false hasContentIssue false
  • English
  • Français

New Young Objects from the IRAS Point Source Catalogue

Published online by Cambridge University Press:  12 April 2016

A. Manchado ,
P. Garcia Lario ,
K. C. Sahu  and
S.R. Pottasch
A. Manchado
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
P. Garcia Lario
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
K. C. Sahu
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands
S.R. Pottasch
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Three new objects have been found, when carrying out a survey of IRAS sources with colours like planetary nebulae, via low resolution spectroscopy. IRAS 14592-6311 and IRAS 07173-1733 are bright cometary nebulae, showing metal line emission very similar to V1331 Cyg (LkHα 120), which is the prototype of a certain number of T Tauri stars. They present strong P-Cygni profiles and some other peculiar characteristics. IRAS 14592-6311 is associated with a molecular cloud at a distance of 2.9 kpc, while IRAS 07173-1733 is located at the edge of the dark cloud KHAV 201. In the case of IRAS 05506+2414, it presents a bipolar structure with Herbig-Haro emission characteristics in one of the lobes, produces by shocked gas, and is located near Orion.

Type
III. Discs, Outflows, Jets and HH Objects
Information
International Astronomical Union Colloquium , Volume 120: Structure and Dynamics of the Interstellar Medium , 1989 , pp. 301
Copyright
Copyright © Springer-Verlag 1989