Zobrazeno 1 - 10
of 1 009
pro vyhledávání: '"infrared : ISM : lines and bands"'
Publikováno v:
Astronomy & astrophysics. 390(3):1089-1113
IR spectroscopy provides a valuable tool for the characterisation and identification of interstellar molecular species. Here, we present 6-9 mum spectra of a sample of reflection nebulae, HII regions, YSOs, evolved stars and galaxies that show strong
Autor:
Aggm Tielens, Els Peeters, Louis J. Allamandola, C. van Kerckhoven, Douglas M. Hudgins, S. Hony, Charles W. Bauschlicher
Publikováno v:
Astronomy & Astrophysics, 390, 1089-1113. EDP Sciences
IR spectroscopy provides a valuable tool for the characterisation and identification of interstellar molecular species. Here, we present 6-9 mum spectra of a sample of reflection nebulae, HII regions, YSOs, evolved stars and galaxies that show strong
Publikováno v:
Astronomy & astrophysics, 380(2), 684-694. EDP Sciences
The ISO and IUE spectra of the elliptical nebulae NGC7662 and NGC6741 are presented. These spectra are combined with the spectra in the visual wavelength region to obtain a complete, extinction corrected, spectrum. The chemical composition of the neb
Publikováno v:
Astronomy & astrophysics. 370(3):1030-1043
We present 10-15 mum spectra of a sample of H II regions. YSOs and evolved stars that show strong unidentified infrared emission features, obtained with the ISO/SWS spectrograph on-board ISO. These spectra reveal a plethora of emission features with
Publikováno v:
Astronomy & astrophysics. 365(3):L353-L356
We report the detection of absorption features in the 6-8 mum region superimposed on a featureless mid-infrared continuum in NGC 4418. For several of these features this is the first detection in an external galaxy We compare the absorption spectrum
Publikováno v:
Astronomy & astrophysics. 365(3):353-356
We report the detection of absorption features in the 6-8 mum region superimposed on a featureless mid-infrared continuum in NGC 4418. For several of these features this is the first detection in an external galaxy We compare the absorption spectrum
Publikováno v:
Astronomy & astrophysics. 363(2):767-778
The ISO and IUE spectra of the bipolar planetary nebulae NGC 6537 and He2-111 are presented. These spectra are combined with the spectrum in the visual wavelength region from the nebulae to obtain a complete spectrum that is corrected for extinction.
Publikováno v:
Astronomy & astrophysics. 360(2):683-698
We have obtained the full 1-200 mu m spectrum of the low luminosity (36 L-circle dot) Class I protostar Elias 29 in the rho Ophiuchi molecular cloud. It provides a unique opportunity to study the origin and evolution of interstellar ice and the inter
Publikováno v:
Astrophysical Journal. 537(2):749-762
We discuss the composition of dust and ice along the line of sight to the Galactic center (GC) based on analysis of mid-infrared spectra (2.4-13 mu m) from the Short Wavelength Spectrometer on the Infrared Space Observatory (ISO). We have analyzed du
Publikováno v:
The Astrophysical Journal. 536(1):347-356
This paper presents, for the first time, a complete 2.4-25 mu m spectrum of the dust-embedded young stellar object W33A. The spectrum was obtained with the Short Wavelength Spectrometer of the Infrared Space Observatory at a mean resolving power of s