2023MNRAS.525..785S


Query : 2023MNRAS.525..785S

2023MNRAS.525..785S - Mon. Not. R. Astron. Soc., 525, 785-804 (2023/October-2)

Orbital period changes for 14 novae and the critical failures of the predictions of standard theories, the Hibernation Model, and the Magnetic Braking Model.

SCHAEFER B.E.

Abstract (from CDS):

The evolution of novae and cataclysmic variables (CVs) is driven by changes in the binary orbital periods. In a direct and critical test for various evolution models and their physical mechanisms, I measure the sudden changes in the period (ΔP) across 14 nova eruptions, and I measure the steady period change during quiescence (Ṗ) for 20 inter-eruption intervals. The standard theory for ΔP is dominated by the mechanism of mass loss, and this fails completely for the five novae with negative values, and it fails to permit the ΔP for U Sco eruptions to change by one order of magnitude eruption to eruption. The Hibernation Model of evolution is refuted because all the ΔP measures are orders of magnitude too small to cause any significant drop in accretion luminosity, and indeed, near half of the nova have negative ΔP as the opposite of the required mechanism for any hibernation state. As for the Magnetic Braking Model, this fails by many orders of magnitude in its predictions of the required Ṗ for 9 out of 13 novae. The observed Ṗ values scatter, both positively and negatively, over a range of ±10–9, while the predicted values are from -10–13 to -10–11. This huge scatter is not possible with standard theory, and there must be some currently unknown mechanism to be added in, with this new mechanism 100-10 000× larger in effect than the current theory allows. In all, these failed predictions demonstrate that nova systems must have unknown physical mechanisms for both ΔP and Ṗ that dominate over all other effects.

Abstract Copyright: © 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): stars: evolution - novae - stars: variables

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 16

goto Full paper

goto View the references in ADS

Number of rows : 16
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 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 V* YZ Ret No* 03 58 29.5511765184 -54 46 41.230757208 15.54 16.588 16.680     sdB?/DA? 76 0
3 V* QZ Aur No* 05 28 34.0779417792 +33 18 21.778535592           ~ 68 0
4 V* T Aur No* 05 31 59.1180488976 +30 26 45.034081044           ~ 291 0
5 V* RR Pic No* 06 35 36.0630266144 -62 38 24.291214934   12.407 12.449 12.675 12.385 ~ 368 0
6 V* BT Mon No* 06 43 47.2416090432 -02 01 13.876883184   15.737 14.638 15.411   G8V 183 0
7 V* T Pyx CV* 09 04 41.5061511720 -32 22 47.502932700           ~ 476 0
8 V* IM Nor No* 15 39 26.4789581496 -52 19 17.968468997           ~ 98 0
9 V* T CrB Sy* 15 59 30.1622265912 +25 55 12.613382940   11.516 10.247 9.70   M3IIIe_sh 810 0
10 V* U Sco CV* 16 22 30.7791646104 -17 52 43.166822628           F8+K2 592 0
11 V* V394 CrA No* 18 00 26.0346757464 -39 00 34.388605836           ~ 139 0
12 V* DQ Her CV* 18 07 30.2510391864 +45 51 32.564791872   14.605 14.443 14.800   M3+Ve 1048 1
13 V* V1017 Sgr No* 18 32 04.4738065392 -29 23 12.593851152       13.479   G5IIIep 149 0
14 UCAC4 443-085347 CV* 18 52 03.5647256952 -01 28 39.190318140       13.373   ~ 176 0
15 V* HR Del No* 20 42 20.3468874528 +19 09 39.305636208   12.380 12.404 12.508   ~ 515 0
16 V* V1500 Cyg No* 21 11 36.5809818696 +48 09 01.952490204           ~ 820 0

To bookmark this query, right click on this link: simbad:objects in 2023MNRAS.525..785S and select 'bookmark this link' or equivalent in the popup menu