Neutral hydrogen associated with the high latitude cloud L 1642

Details Neutral hydrogen associated with the high latitude cloud L 1642 Neutral hydrogen associated with the high latitude cloud L 1642

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...196..243l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 196, no. 1-2, May 1988, p. 243-251. Research supported by the Academy of Finla

Astronomy and Astrophysics

Astrophysics

17

B Stars, Hydrogen Clouds, Molecular Clouds, Nebulae, O Stars, Stellar Radiation, Brightness Temperature, Interstellar Gas, Line Spectra, Neutral Gases, Thermal Emission, Ultraviolet Radiation

Scientific paper

The 100-m radio telescope at Effelsberg was used to map the high-galactic-latitude (b = - 36.7 deg) dark nebula Lynds 1642 in the 21-cm H I line. In the central part of L 1642, the radial velocity of the H I line is in good agreement with different molecular line velocities of L 1642 in the range of 0 to 1.0 km/s. The line width map of H I reveals an increase from 2.5 to 2.9 km/s over a small area on the 'bright side' of L 1642.

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