High Rydberg State Carbon Recombination Lines from Interstellar Clouds

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dc.creatorAnantharamaiah, K. R.
dc.creatorKantharia, Nimisha G.
dc.date1999-03-03
dc.date.accessioned2026-07-07T02:30:41Z
dc.date.available2026-07-07T02:30:41Z
dc.descriptionWe report observations of carbon recombination lines near 34.5 MHz (qunatum number n=578) and 325 MHz (n=272) made towards Cas A, the Galactic centre and about ten other directions in the galactic plane. Constraints on the physical conditions in the line forming regions are derived from these and other existing observations. The CII regions that produce the low-frequency lines are most likely associated with the neutral HI component of the ISM.
dc.description4 pages, 3 figures; Presented at the workshop on "New Perspects on the Interstellare Medium", Penticton, Canada, Aug 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9903076
dc.identifierhttp://arxiv.org/abs/astro-ph/9903076
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13896
dc.subjectAstrophysics
dc.titleHigh Rydberg State Carbon Recombination Lines from Interstellar Clouds
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