Wide field imaging of the star forming region Lynds 1551.

Details Wide field imaging of the star forming region Lynds 1551. Wide field imaging of the star forming region Lynds 1551.

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..24...99g&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 24, No. 1, p. 99 - 107

Astronomy and Astrophysics

Astronomy

16

Scientific paper

The authors have obtained images of the L1551 star forming region using narrow band filters centered on the Hα and [S II] 6717/31 emission lines. Many of the semi-stellar knots recently discovered in this zone by Graham and Heyer (1990) in their Hα+[N II] images have very strong [S II] emission. Their structure and emission suggest that these are Herbig-Haro objects. HH 30, at ≡4 arcminutes NE of IRS 5, has a detectable counterjet in the Hα images, but it is absent in the [S II] images. The authors suggest that the HH 30 counterjet may be interacting with the L1551 cavity near the reflection nebula in HH 102.

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