The infrared spectrum of Gamma Velorum
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 200 (1982) 69P-75P-69P-75P
Abstract:
Infrared spectral observations of the Wolf-Rayet system Gamma Velorum in the atmospheric windows between 1.45 and 12 microns are presented. Results show an extremely rich emission line spectrum in which permitted lines of helium and carbon and forbidden lines of neon and sulfur are present, some of which have not previously been observed in any object. The relative abundances of He I/He II and C/He are estimated, and lower limits to the Ne/He and S/He abundance ratios are presented.8-13 micron spectrophotometry of compact planetary nebulae and emission line objects
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 200 (1982) 217-237-217-237
Abstract:
8-13 micron spectra are presented of 24 planetary nebulae and other emission line objects, 19 of which are published here for the first time. This brings the total of planetary nebulae for which such spectra are available to 23 including four classed as very low excitation (VLE) objects and three as WC-11 objects. On the basis of these spectra, roughly one-third of the planetaries are identified as having oxygen-rich (silicate) and rather less than one-third carbon-rich (silicon carbide) dust grains. Of the oxygen-rich nebulae, three are VLEs while the rest are very compact and, on various grounds, considered to be young. The remainder of the planetary nebulae exhibit strongly the unidentified feature at 11.25 microns and frequently that at 8.65 microns and their dust chemistry is uncertain. All of the 23 planetaries exhibit one or more of the fine structure forbidden lines of Ar III, S IV and Ne II roughly in accordance with their optical excitation class. The line intensities are consistent with approximately solar abundance of these elements.A high-excitation optically obscured H II region in the nucleus of NGC 5253
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 199 (1982) 31P-35P
Abstract:
Spectrophotometry from 8-13 microns of the strong infrared source in the nucleus of NGC 5253 indicates the presence of an obscured region of very high ionization. The shape of the dust continuum suffering from silicate absorption and the strength of the forbidden lines S IV fine structure line require either a compact cluster of several hundred early O stars or a single massive highly luminous object within 50 pc of the nucleus obscured in the visible, to provide both the infrared luminosity and ionizing flux. It appears that the infrared emission has been produced by a recent burst of star formation, probably with a bias towards more massive stars, and the 8-13 micron spectrum shows no evidence for the narrow emission features of 11.25 and 8.65 microns, or the forbidden lines Ne II line at 12.8 microns.Spatial and spectral studies of the Galactic center near 10 μm
AIP Conference Proceedings AIP (1982)
The question of extinction in active galactic nuclei - Infrared spectral observations of NGC 1614, NGC 7469 and NGC 1275
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 196 (1981) 101P-107P-101P-107P