Authors:
López R., Rosado M., Riera A., Noriega-Crespo A., Raga A.C., Estalella R., Anglada G., Le Coarer E., Langarica R., Tinoco S., Cantó J.
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 Å 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.
Keywords:
Individual (HH 262, L1551 IRS 5) - ISM; ISM; Jets and outflows