Observations Towards Star Formation Regions: H2 Near-Infrared Emission Lines

Details Observations Towards Star Formation Regions: H2 Near-Infrared Emission Lines Observations Towards Star Formation Regions: H2 Near-Infrared Emission Lines

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..201p&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 201-204 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present near-infrared images of HH93 and L1251. The detection of
H2 emission allows us to study deeply embedded shocks,
produced by the strong winds of young stars.

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