Hostname: page-component-7479d7b7d-t6hkb Total loading time: 0 Render date: 2024-07-11T06:28:47.365Z Has data issue: false hasContentIssue false

Observations of the 126α Line of Excited Hydrogen in Southern HII Regions

Published online by Cambridge University Press:  25 April 2016

F. F. Gardner
Affiliation:
Division of Radiophysics, CSIRO, Sydney
R. X. McGee
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

A search for the 126a hydrogen recombination line, with a rest frequency of 3248.713 MHz, has been made in the 19 sources listed in Table I using the Parkes telescope. The beamwidth was 6′ are and the frequency resolution 37 kHz. In the Table RCW refers to the Rodgers, Campbell and Whiteoak Atlas, W to the Westerhout catalogue, and the co-ordinate numbers to the Parkes Catalogue of Sources. In each case the ratio of the peak of the line to the continuum TL/TC, the half-intensity width Δv and the mean radial velocity to the local standard of rest, were determined. The related velocities observed in OH emission and absorption are also shown.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1967

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Hoglund, B., and Mezger, P. C., 1965.—Science, 150, 339.Google Scholar
2 Kardashev, N. S., 1960.—Soviet AJ., 3, 813.Google Scholar
3 Goldberg, L., 1966.—Ap. J., 144, 1225.Google Scholar