Evidence from sub-millimetre observations for thermal dust emission in NGC4151
- 1 December 1988
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 336 (6201) , 749-751
- https://doi.org/10.1038/336749a0
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- The submillimeter spectral break in Seyfert galaxiesThe Astrophysical Journal, 1988
- The infrared diagnostic of a dusty plasma with applications to supernova remnantsThe Astrophysical Journal, 1987
- Millimeter-wave spectra and variability of bright, compact radio sourcesThe Astronomical Journal, 1987
- Broad-band properties of the CfA Seyfert Galaxies. II - Infrared to millimeter propertiesThe Astrophysical Journal, 1987
- A detailed study of the C IV 1550-A line profile and adjacent spectral features in NGC 4151 from 1978 to 1983The Astrophysical Journal, 1987
- The continuum of type 1 Seyfert galaxies. II - Separating thermal and nonthermal componentsThe Astrophysical Journal, 1987
- Far-infrared properties of optically selected quasarsThe Astrophysical Journal, 1986
- Spectral energy distributions of active galactic nuclei between 0.1 and 100 micronsThe Astrophysical Journal, 1986
- Submillimeter and millimeter observations of Uranus and NeptuneIcarus, 1986
- Variability and the nature of QSO optical-infrared continuaThe Astrophysical Journal, 1985