2023RNAAS...7..191S

Query : 2023RNAAS...7..191S

2023RNAAS...7..191S - Research Notes of the AAS, 7, 191 (2023/September-0)

Concerning the Verity of the MMRD Relation for Novae.

SHAFTER A.W., CLARK J.G. and HORNOCH K.

Abstract (from CDS):

It has long been claimed that novae reaching the highest luminosity at the peak of their eruptions appear to fade the fastest from maximum light. The relationship between peak brightness and fade rate is known as the Maximum-Magnitude, Rate-of-Decline (MMRD) relation. Lightcurve parameters for the most recent sample of M31 recurrent novae are presented and used to buttress the case that the observed MMRD relation can be explained as a consequence of observational selection effects coupled with expectations from standard nova models.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Cataclysmic variable stars - Novae - Recurrent novae

Simbad objects: 23

goto Full paper

goto View the references in ADS

Number of rows : 23
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 SV* SON 10729 No* 00 39 30.80 +40 29 15.0           ~ 5 0
2 M31N 2007-11f No* 00 41 31.52 +41 07 13.1           ~ 7 0
3 PNV J00413317+4110124 No* 00 41 33.17 +41 10 12.4           ~ 9 0
4 AT 2021rno No* 00 42 38.37 +41 08 45.8     17.50     ~ 9 0
5 AT 2021vgi No* 00 42 39.59 +41 09 04.0           ~ 22 0
6 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
7 EV* M31 V0922 No* 00 42 47.15 +41 16 19.8     17.60 17.9   ~ 21 0
8 M31N 1926-07c No* 00 42 53.37 +41 15 43.7     18.20     ~ 13 0
9 Rosino 29 No* 00 42 55.66 +41 14 11.7     16.90     ~ 18 0
10 AT 2020yug No* 00 42 57.74 +41 08 12.1     17.30     ~ 40 0
11 M31N 1990-10a No* 00 43 04.05 +41 17 07.5           ~ 22 0
12 AT 2017jdm No* 00 43 29.50 +41 17 13.0       17.8   ~ 14 0
13 TCP J00441072+4154221 No* 00 44 10.72 +41 54 22.1           ~ 13 0
14 RX J0045.4+4154 No* 00 45 28.80 +41 54 10.1           ~ 263 1
15 V* T Pyx CV* 09 04 41.5061511720 -32 22 47.502932700           ~ 476 0
16 V* IM Nor No* 15 39 26.4789581496 -52 19 17.968468997           ~ 98 0
17 V* T CrB Sy* 15 59 30.1622265912 +25 55 12.613382940   11.516 10.247 9.70   M3IIIe_sh 810 0
18 V* U Sco CV* 16 22 30.7791646104 -17 52 43.166822628           F8+K2 592 0
19 V* V2487 Oph No* 17 31 59.805 -19 13 56.13   18.0       ~ 136 0
20 V* V745 Sco Sy* 17 55 22.2260994408 -33 14 58.551839808     17.987   13.353 M2/M6IIIe 265 1
21 V* V394 CrA No* 18 00 26.0346757464 -39 00 34.388605836           ~ 139 0
22 V* V3890 Sgr No* 18 30 43.2877623168 -24 01 08.944843980     15.944 14.798 12.611 M5III 232 0
23 UCAC4 443-085347 CV* 18 52 03.5647256952 -01 28 39.190318140       13.373   ~ 176 0

To bookmark this query, right click on this link: simbad:objects in 2023RNAAS...7..191S and select 'bookmark this link' or equivalent in the popup menu