Near-infrared CO emission in young stellar objects ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

IRAS CPC observations of a region measuring 25× 25 arcmin2 in the NGC 1333 molecular
cloud have revealed nine distinct far-infrared sources, many of which have not previously …

High-angular resolution molecular hydrogen (H2) v= 1-0 S (1) line images of several well-
known molecular outflow sources (DR 21, NGC 2071, HH 7-11, and HH 12) are presented. It …

A comprehensive model for molecular hydrogen emssion in Herbig-Haro objects that are
associated with the heads of radiative stellar jets is presented by using a simple …

The authors report the results of extensive mapping of the region around SSV 13 in the NGC
1333 star forming region in the CO and 13 CO (J= 1-0) lines at high angular resolution with …

We present infrared echelle spectroscopy of three Herbig-Haro (HH) driving sources (SVS
13, B5-IRS 1, and HH 34 IRS) using Subaru IRCS. The large diameter of the telescope and …

Molecular hydrogen and optical images of HH 7-11 ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

NGC 1333 is the currently most active region of star formation in the Perseus molecular
cloud. The presence of emission-line stars and Herbig-Haro objects first established NGC …

Five emission lines of molecular hydrogen, with wavelengths in the ranges of 2.10–2.25 and
3.80–3.85 μ m, have been observed in four objects of different type in which the line …

We perform a detailed shock diagnosis of the Herbig—Haro object HH7, a well-defined bow
shock from a protostellar outflow. We first present molecular hydrogen images in the 2-1 S …