Closed wkerzendorf closed 13 years ago
Thanks brian. but they are very similar otherwise? I mean why do the IIL's not have the hydrogen recombination phase like the IIPs? Not enough hydrogen?
They have some recombination phase, but the energy scales are such that it doesn't matter as much as other things.
On 3/05/11 11:04 PM, wkerzendorf wrote:
Thanks brian. but they are very similar otherwise? I mean why do the IIL's not have the hydrogen recombination phase like the IIPs? Not enough hydrogen?
Professor Brian P. Schmidt Telephone: 61 (0)2 6125 8042 ARC Laureate Fellow Fax: 61 (0)2 6125 0260 ANU Distinguished Professor The Australian National University Mt Stromlo Observatory The Research School of Astronomy and Astrophysics Weston Creek, ACT 2611 Australia
II-L is a SN like 1980K and 1979C which are hydrogen rich, and decline monotonically from maximum light without a plateau
Ibc are hydrogen deficient massive stellar explosions.
On 3/05/11 6:02 PM, wkerzendorf wrote:
Professor Brian P. Schmidt Telephone: 61 (0)2 6125 8042 ARC Laureate Fellow Fax: 61 (0)2 6125 0260 ANU Distinguished Professor The Australian National University Mt Stromlo Observatory The Research School of Astronomy and Astrophysics Weston Creek, ACT 2611 Australia