2010ApJS..187..275S


C.D.S. - SIMBAD4 rel 1.7 - 2019.10.17CEST03:04:03

2010ApJS..187..275S - Astrophys. J., Suppl. Ser., 187, 275-373 (2010/April-0)

Comprehensive photometric histories of all known galactic recurrent novae.

SCHAEFER B.E.

Abstract (from CDS):

I collect virtually all photometry of the 10 known galactic recurrent novae (RNe) and their 37 known eruptions. This consists of my modern measures of nearly all archival plates (providing the only data for half of 37 known eruptions), my own 10,000 CCD magnitudes from 1987 to present (providing virtually all of the magnitudes in quiescence for seven RNe), over 140,000 visual magnitude estimates recorded by amateur astronomers (who discovered half the known eruptions), and the small scattering of magnitudes from all the literature. From this, I produce various uniform products: (1) BVRIJHK comparison star magnitudes and BV comparison star sequences to cover the entire range of eruption; (2) complete light curves for all eruptions; (3) best-fit B and V light curve templates; (4) orbital periods for all but one RN; (5) exhaustive searches for all missed eruptions; (6) measured discovery efficiencies since 1890; (7) true recurrence time scales; (8) predicted next eruption dates; (9) variations on time scales of minutes, hours, days, months, years, decades, and century; (10) uniform distances and extinctions to all RNe; (11) BV colors at peak and UBVRIJHK colors at minimum, all with extinction corrections; and (12) the spectral energy distributions over UBVRIJHK. Highlights of this work include the discoveries of one new RN, six previously unknown eruptions, and the orbital periods for half the RNe. The goal of this work is to provide uniform demographics for answering questions like the "What is the death rate of RNe in our Galaxy?" and "Are the white dwarfs gaining or losing mass over each eruption cycle?" An important use of this work is for the question of whether RNe can be the progenitors of Type Ia supernovae.

Abstract Copyright:

Journal keyword(s): novae, cataclysmic variables - stars: individual (T Pyx, U Sco, CI Aql, RS Oph, V2487 Oph)

VizieR on-line data: <Available at CDS (J/ApJS/187/275): novae.dat table4.dat table5.dat table22.dat>

Simbad objects: 36

goto Full paper

goto View the reference in ADS

Number of rows : 36

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 * omi Cet Mi* 02 19 20.79210 -02 58 39.4956   7.63 6.53 5.03   M5-9IIIe+DA 1412 0
2 V* GK Per No* 03 31 12.0096626899 +43 54 15.467450081   10.2 14.0     K1IV 859 0
3 SN 1987A SN* 05 35 28.020 -69 16 11.07   4.75 4.81     SN.IIPec 4382 2
4 NOVA Ori 1667 No* 05 58 20.1459511355 +20 15 45.348138439     6.0     ~ 23 0
5 1A 0620-00 HXB 06 22 44.5420315454 -00 20 44.289428950 10.60 11.40 11.2     K3V-K7V 1029 0
6 HD 77897 * 09 04 18.0905927616 -31 50 39.939817417   10.34 10.25     B9IV 3 0
7 NOVA Pyx 1890 No* 09 04 41.5062068236 -32 22 47.503345173   7.0       ~ 375 1
8 CD-31 6884 * 09 04 45 -32 25.6           ~ 1 0
9 CD-31 6903 * 09 05 34.8500498190 -32 20 28.341012170   10.66 10.11     ~ 2 0
10 NAME Car Arm PoG 10 00 -60.0           ~ 367 1
11 V* RZ Leo DN* 11 37 22.2523056583 +01 48 58.617841432     19.6     DA+dM2 144 0
12 SN 1974G SN* 12 26 28 +31 12.4   12.48       SNIa 94 1
13 SN 1960F SN* 12 31 42.05 +03 56 47.7   11.34 11.43     SNIa 111 1
14 SN 1981B SN* 12 34 29.57 +02 11 59.3   11.74       SNIa 381 1
15 SN 1937C SN* 13 05 53.2 +37 36 07   8.80 8.77     SNIa 199 1
16 NOVA Nor 1920 No* 15 39 26.465 -52 19 17.99           ~ 76 0
17 V* T CrB Sy* 15 59 30.1619486506 +25 55 12.607985109 2.69 2.10 2.00     M3III+p 637 0
18 HD 144287 SB* 16 04 03.6358576495 +25 15 17.167593790   7.87   6.6   G8+V 150 0
19 NOVA Sco 1863 No* 16 22 30.7782086963 -17 52 43.162570042   8.80 8.70     F8+K2 458 0
20 V* V1195 Oph DN* 17 00 21.67 -20 53 34.4           ~ 16 0
21 V* V2487 Oph No* 17 31 59.805 -19 13 56.13   18.0       ~ 100 0
22 V* RS Oph No* 17 50 13.1592776879 -06 42 28.481553668   12.29 4.30     OB+M2ep 906 0
23 V* V745 Sco LP* 17 55 22.2273446574 -33 14 58.558723074     17.987   13.353 ~ 180 0
24 NOVA CrA 1987 No* 18 00 25.97 -39 00 35.1           ~ 122 0
25 V* V533 Her No* 18 14 20.4845602013 +41 51 22.070248280           ~ 231 0
26 V* V3890 Sgr LP* 18 30 43.2881019064 -24 01 08.948570280   13.5 15.944   12.611 ~ 121 0
27 V* V1017 Sgr No* 18 32 04.4737964965 -29 23 12.593546512           G5IIIp 122 0
28 NOVA Aql 1917 No* 18 52 03.5647265171 -01 28 39.191180908           ~ 144 0
29 V* V446 Her No* 18 57 21.5917264330 +13 14 29.319279140           ~ 128 0
30 KPD 1930+2752 HS* 19 32 14.8086352823 +27 58 35.444970697 12.80 13.75 13.82     sdB 142 0
31 V* WZ Sge DN* 20 07 36.5036203067 +17 42 14.733657651   15.30 15.20     DAepv 885 0
32 V* PU Vul No* 20 21 13.3112218215 +21 34 18.693825946   11.13 10.87     A4II-F8Iab+M6IIIe 291 0
33 V* V1500 Cyg No* 21 11 36.5811336631 +48 09 01.950330133   17.9       ~ 736 0
34 V* VY Aqr DN* 21 12 09.2516769018 -08 49 36.776018749   8.00       ~ 210 1
35 V* Q Cyg No* 21 41 43.9276952364 +42 50 29.039173205           ~ 106 0
36 NAME Local Group GrG ~ ~           ~ 6658 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2010ApJS..187..275S and select 'bookmark this link' or equivalent in the popup menu


2019.10.17-03:04:04

© Université de Strasbourg/CNRS

    • Contact