SIMBAD references

2001A&A...372..165M - Astronomy and Astrophysics, volume 372, 165-172 (2001/6-2)

The complete ISO spectrum of NGC 6302.

MOLSTER F.J., LIM T.L., SYLVESTER R.J., WATERS L.B.F.M., BARLOW M.J., BEINTEMA D.A., COHEN M., COX P. and SCHMITT B.

Abstract (from CDS):

We present the combined Infrared Space Observatory Short-Wavelength Spectrometer and Long-Wavelength Spectrometer 2.4-197µm spectrum of the Planetary Nebula NGC 6302 which contains in addition to strong atomic lines, a series of emission features due to solid state components. The broad wavelength coverage enables us to more accurately identify and determine the properties of both oxygen- and carbon-rich circumstellar dust. A simple model fit was made to determine the abundance and typical temperature of the amorphous silicates, enstatite and forsterite. Forsterite and enstatite do have roughly the same abundance and temperature. The origin and location of the dust in a toroidal disk around the central star are discussed.

Abstract Copyright:

Journal keyword(s): circumstellar matter: planetary nebulae: individual: NGC 6302 - infrared: ISM: lines and bands

CDS comments: in ref list Ashley 1988ApJ...331..532A instead of 331.582, Gomez 1993ApJ...416..620G instead of ApJ...416.420

Simbad objects: 5

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2001A&A...372..165M and select 'bookmark this link' or equivalent in the popup menu


2020.09.28-21:56:18

© Université de Strasbourg/CNRS

    • Contact