HH 262: The red lobe of the L1551 IRS 5 outflow

DOI: 
10.1086/300455
Publication date: 
01/08/1998
Main author: 
Lopez, R
IAA authors: 
Authors: 
Lopez, R; Rosado, M; Riera, A; Noriega-Crespo, A; Raga, AC; Estalella, R; Anglada, G; Le Coarer, E; Langarica, R; Tinoco, S; Canto, J
Journal: 
ASTRONOMICAL JOURNAL
Publication type: 
Article
Volume: 
116
Pages: 
845-853
Number: 
Abstract: 
HH 262 is a group of emitting knots located approximately 3.'5 to the northeast of the L1551 IRS 5 source. We present a detailed study of the kinematic properties of HH 262, based on proper-motion measurements and on high-resolution imaging Fabry-Perot observations in the [S II] 6717 Angstrom line. From these observations, we conclude that it indeed appears to be the case that HH 262 is associated with the red lobe of the L1551 IRS 5 outflow.
Database: 
WOK
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/1998AJ....116..845L/abstract
ADS Bibcode: 
1998AJ....116..845L
Keywords: 
ISM : individual (HH 262, L1551 IRS 5); ISM : jets and outflows