A PHYSICAL MODEL FOR SN 2001ay, A NORMAL, BRIGHT, EXTREMELY SLOW DECLINING TYPE Ia SUPERNOVA
dc.creator | Baron, E. | |
dc.creator | Höflich, P. | |
dc.creator | Krisciunas, K. | |
dc.creator | Dominguez, I. | |
dc.creator | Khokhlov, A. M. | |
dc.creator | Phillips, M. M. | |
dc.creator | Suntzeff, N. | |
dc.creator | Wang, L. | |
dc.date.accessioned | 2019-10-09T16:22:51Z | |
dc.date.available | 2019-10-09T16:22:51Z | |
dc.date.issued | 2012 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.issn | 1538-4357 | |
dc.identifier.uri | https://hdl.handle.net/1969.1/180694 | |
dc.format.extent | 1 | en |
dc.publisher | The Astrophysical Journal | |
dc.relation.ispartof | 1foldr Import 2019-10-08 Batch 5 | en |
dc.relation.uri | 10.1088/0004-637X/753/2/105 | en |
dc.title | A PHYSICAL MODEL FOR SN 2001ay, A NORMAL, BRIGHT, EXTREMELY SLOW DECLINING TYPE Ia SUPERNOVA | en |