M31N 2007-11d: A Slowly-Rising, Luminous Nova in M31
| dc.creator | Shafter, A. W. | |
| dc.creator | Rau, A. | |
| dc.creator | Quimby, R. M. | |
| dc.creator | Kasliwal, M. M. | |
| dc.creator | Bode, M. F. | |
| dc.creator | Darnley, M. J. | |
| dc.creator | Misselt, K. A. | |
| dc.date | 2008-09-08 | |
| dc.date.accessioned | 2026-07-07T12:15:35Z | |
| dc.date.available | 2026-07-07T12:15:35Z | |
| dc.description | We report a series of extensive photometric and spectroscopic observations of the luminous M31 nova M31N 2007-11d. Our photometric observations coupled with previous measurements show that the nova took at least four days to reach peak brightness at R~14.9 on 20 Nov 2007 UT. After reaching maximum, the time for the nova to decline 2 and 3 magnitudes from maximum light (t_2 and t_3) was ~9.5 and ~13 days, respectively, establishing that M31N 2007-11d was a moderately fast declining nova. During the nova's evolution a total of three spectra were obtained. The first spectrum was obtained one day after maximum light (5 days post-discovery), followed by two additional spectra taken on the decline at two and three weeks post-maximum. The initial spectrum reveals narrow Balmer and Fe II emission with P Cygni profiles superimposed on a blue continuum. These data along with the spectra obtained on the subsequent decline clearly establish that M31N 2007-11d belongs to the Fe II spectroscopic class. The properties of M31N 2007-11d are discussed within the context of other luminous novae in M31, the Galaxy, and the LMC. Overall, M31N 2007-11d appears to be remarkably similar to Nova LMC 1991, which was another bright, slowly-rising, Fe II nova. A comparison of the available data for luminous extragalactic novae suggest that the >~4 day rise to maximum light seen in M31N 2007-11d may not be unusual, and that the rise times of luminous Galactic novae, usually assumed to be <~2 days, may have been underestimated. | |
| dc.description | Accepted for publication in The Astrophysical Journal (28 pages, 6 figures) | |
| dc.identifier | https://arxiv.org/abs/0809.1388 | |
| dc.identifier | http://arxiv.org/abs/0809.1388 | |
| dc.identifier | Astrophys.J.690:1148-1157,2009 | |
| dc.identifier | doi:10.1088/0004-637X/690/2/1148 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/211531 | |
| dc.subject | Astrophysics | |
| dc.title | M31N 2007-11d: A Slowly-Rising, Luminous Nova in M31 | |
| dc.type | text |