The moderate spatial resolution and high sensitivity of the Infrared Astronomical Satellite (IRAS), which surveyed the celestial sphere during 1983 at wavelengths of 12, 25, 60, and 100 microns, were particularly well suited to detecting extended thermal emission from cometary dust. Sources with infrared color temperatures characteristic of solar system bodies, and at the ephemerides position of known comets were selected for analysis by the IRAS Asteroid Data Analysis System (ADAS). The data base is now available for use by researchers. This paper describes the development of the data base, details its entries, and presents a statistical analysis of its contents. The IRAS survey contains multiple observations of many periodic comets. A brief description and analysis is given of the observed infrared and derived physical properties for several comets of special interest.


    Access

    Access via TIB

    Check availability in my library


    Export, share and cite



    Title :

    IRAS observations of comets


    Contributors:

    Published in:

    Publication date :

    1986-01-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English


    Keywords :


    IRAS observations of comets

    Walker, R.G. / Matson, D.L. / Veeder, G.J. | Elsevier | 1987


    Recent infrared observations of comets with UKIRT and IRAS

    Zarnecki, J.C. / McDonnell, J.A.M. / Carey, W.C. et al. | Elsevier | 1984


    IRAS observations of cometary dust

    Walker, R. G. / Aumann, H. H. | NTRS | 1984


    IRAS observations of cometary dust

    Walker, R.G. / Aumann, H.H. | Elsevier | 1984


    IRAS observations of the zodiacal background

    Good, J.C. / Hauser, M.G. / Gautier, T.N. | Elsevier | 1987