Observations of SN 1987A in the mid-infrared.
Abstract
Mid-IR (5-30 microns) observations of SN 1987A are reviewed. The ionic masses of Co I, Co II, Ni I, Cl I, Ne II and Ni-56 are estimated from the line intensities. It is found that, one year after the explosion, the velocities appropriate to the hydrogenic and ionic regions are about 2000 km/s and 1500 km/s, respectively. An ionization fraction of a few percent is derived for the hydrogen/helium envelope. It is suggested that the appearance of neutral ions at 15 months may indicate that dust formation may be imminent.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- 1988
- DOI:
- Bibcode:
- 1988PASA....7..462A
- Keywords:
-
- Infrared Spectroscopy;
- Spectrum Analysis;
- Stellar Composition;
- Stellar Spectra;
- Supernova 1987a;
- Continuous Spectra;
- Emission Spectra;
- Forbidden Transitions;
- Line Spectra;
- Astrophysics