Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-13T05:53:24.998Z Has data issue: false hasContentIssue false
  • English
  • Français

New Observational Near-Infrared Spectroscopic Results on Several IRAS Sources with Emission Features

Published online by Cambridge University Press:  04 August 2017

M. De Muizon ,
L.B. D'Hendecourt ,
T. R. Geballe ,
F. Baas  and
C. Perrier
M. De Muizon
Affiliation:
Sterrewacht Leiden Postbus 9513, 2300 RA Leiden, Netherlands
L.B. D'Hendecourt
Affiliation:
Sterrewacht Leiden Postbus 9513, 2300 RA Leiden, Netherlands
T. R. Geballe
Affiliation:
Sterrewacht Leiden Postbus 9513, 2300 RA Leiden, Netherlands
F. Baas
Affiliation:
Sterrewacht Leiden Postbus 9513, 2300 RA Leiden, Netherlands
C. Perrier
Affiliation:
Sterrewacht Leiden Postbus 9513, 2300 RA Leiden, Netherlands

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have obtained spectra in the three micron region of a sample of IRAS sources showing a strong 11.3 micron emission feature in their IRAS Low-Resolution Spectra (LRS). The observations have been carried out from ESO (La Silla, Chile) and from UKIRT (Mauna Kea, Hawaii), between March and September 1985. All sources but one turn out to have a more or less strong 3.3 micron emission feature, and additionally in most cases a feature at 3.4 micron, extending into a plateau from 3.45 to 3.60 micron. in one particular case we have resolved the plateau into 3 features at 3.45, 3.51 and 3.56 micron. These are detected for the first time.

Type
Grains
Information
Symposium - International Astronomical Union , Volume 120: Astrochemistry , 1987 , pp. 555
Copyright
Copyright © Reidel 1987