Published February 15, 1982 | Version v1
Journal article

High spectral and spatial resolution observations of the 12.28 Micron emission from H2 in the Orion Molecular Cloud

  • 1. Department of Physics, University of California, Berkeley

Description

The pure rotational S(2) line of molecular hydrogen at 12.28 μm has been looked for in 44 positions in the Orion Molecular Cloud with 6' beams and 35 km s-1 spectral resolution; it was detected in 27 positions. Emission has been observed over a velocity range of +- 100 km s-1. The lines are approximately symmetric and have full widths at half-maximum ranging from 100 km s-1 down to the resoluton limit. The distribution of intensities and line shapes is largely consistent with that seen in the 2 μm hydrogen transitions. However, unexpectedly complex line profiles and point-to-point variations in the line shapes appear, particularly in the region near IRc9

Additional details

Publishing Information

Journal Title
Astrophys. J., Lett. Ed.
Journal Volume
253
Journal Issue
2
Series
Astrophys. J., Lett. Ed.
Journal Page Range
L83-L87
ISSN
0571-7248

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
14722397
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
EMISSION SPECTRA; HYDROGEN; INFRARED SPECTRA; INTERSTELLAR SPACE; MOLECULES; NEBULAE; ROTATIONAL STATES; SPECTRAL FUNCTIONS
Descriptors DEC
ELEMENTS; ENERGY LEVELS; EXCITED STATES; FUNCTIONS; NONMETALS; SPACE; SPECTRA