A radio continuum and H i study of IC 63, IC 59, and IRAS 00556 + 6048: nebulae in the vicinity of γ Cas | Zendy

D. Blouin | Zendy; W. H. McCutcheon | Zendy; P. E. Dewdney | Zendy; R. S. Roger | Zendy; C. R. Purton | Zendy; D. J. M. Kester | Zendy; Tj. R. Bontekoe | Zendy

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A radio continuum and H i study of IC 63, IC 59, and IRAS 00556 + 6048: nebulae in the vicinity of γ Cas

Author(s) -

D. Blouin,

W. H. McCutcheon,

P. E. Dewdney,

R. S. Roger,

C. R. Purton,

D. J. M. Kester,

Tj. R. Bontekoe

Publication year - 1997

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/287.2.455

Subject(s) - physics , astrophysics , infrared , ionization , h ii region , telescope , emission spectrum , molecular cloud , photodissociation , star formation , astronomy , stars , spectral line , ion , chemistry , photochemistry , quantum mechanics

Sh 185, which is associated with the B0-B0.5IV star γ Cas and contains the two nebulae IC 63 and IC 59, has been observed with the DRAO synthesis telescope in continuum emission at 408 and 1420 MHz, and in H I line emission. Continuum emission is clearly detected for IC 63 and weakly detected for IC 59. The emission from both nebulae is thermal, with the masses of ionized gas being 0.08 and 0.07 M...

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