HH 262: The Red Lobe of the L1551 IRS 5 Outflow

Details HH 262: The Red Lobe of the L1551 IRS 5 Outflow HH 262: The Red Lobe of the L1551 IRS 5 Outflow

Aug 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aj....116..845l&link_type=abstract

The Astronomical Journal, Volume 116, Issue 2, pp. 845-853.

Astronomy and Astrophysics

Astronomy

10

Ism: Individual (Hh 262, L1551 Irs 5), Ism: Jets And Outflows

Scientific paper

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.

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