HH-262 - THE RED LOBE OF THE L1551 IRS-5 OUTFLOW

Authors
LOPEZ R ROSADO M RIERA A NORIEGACRESPO A RAGA AC ESTALELLA R ANGLADA G LECOARER E LANGARICA R TINOCO S CANTO J
Citation
R. Lopez et al., HH-262 - THE RED LOBE OF THE L1551 IRS-5 OUTFLOW, The Astronomical journal (New York), 116(2), 1998, pp. 845-853
Citations number
27
Categorie Soggetti
Astronomy & Astrophysics
Journal title
The Astronomical journal (New York) → ACNP
ISSN journal
00046256
Volume
116
Issue
2
Year of publication
1998
Pages
845 - 853
Database
ISI
SICI code
0004-6256(1998)116:2<845:H-TRLO>2.0.ZU;2-N
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 th e 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 indee d appears to be the case that HH 262 is associated with the red lobe o f the L1551 IRS 5 outflow.