2015A&A...576A.119T

Query : 2015A&A...576A.119T

2015A&A...576A.119T - Astronomy and Astrophysics, volume 576A, 119-119 (2015/4-1)

SALT observations of southern post-novae.

TOMOV T., SWIERCZYNSKI E., MIKOLAJEWSKI M. and ILKIEWICZ K.

Abstract (from CDS):

We report on recent optical observations of the stellar and the nebular remnants of 22 southern post-novae. In this study, for each of our targets, we obtained and analysed long-slit spectra in the spectral range 3500-6600Å and in Hα+[NII] narrow-band images. The changes in the emission lines' equivalent widths with the time since the outburst agree with earlier published results of other authors. We estimated an average value α=2.37 for the exponent of the power law fitted to the post-novae continua. Our observations clearly show the two-component structure of the V842 Cen expanding nebulae, owing to the different velocities of the ejected matter. We discovered an expanding shell around V382 Vel with an outer diameter of about 12''.

Abstract Copyright: ∼

Journal keyword(s): novae, cataclysmic variables

Simbad objects: 36

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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 - 2024 		#notes
1 CPD-69 177 WD* 03 10 31.0195960176 -68 36 03.380768388 10.757 11.413 11.394 11.47 11.558 DA3.0 264 0
2 V* V529 Ori CV* 05 58 20.1408457344 +20 15 45.369052992           ~ 25 0
3 V* RR Pic No* 06 35 36.0630266144 -62 38 24.291214934   12.407 12.449 12.675 12.385 ~ 350 0
4 V* BT Mon No* 06 43 47.2416090432 -02 01 13.876883184   15.737 14.638 15.411   G8V 174 0
5 HD 289002 * 06 45 13.3725491952 +02 08 14.685250596 10.06 10.62 10.44     B1 259 0
6 V* GI Mon No* 07 26 47.1066965424 -06 40 29.708015988           ~ 55 0
7 V* V445 Pup No* 07 37 56.8797787992 -25 56 58.837610328       13.654 12.849 ~ 179 0
8 V* HS Pup No* 07 53 24.8917786080 -31 38 50.564032260           ~ 28 0
9 V* HZ Pup No* 08 03 22.8480059616 -28 28 28.556335236       15.008   ~ 47 0
10 V* CP Pup No* 08 11 46.0634106720 -35 21 04.986480708   15.436 15.227     ~ 264 1
11 V* DY Pup CV* 08 13 48.4791397056 -26 33 56.772073116   19.0   19.0 18.45 ~ 28 0
12 V* Z Cam CV* 08 25 13.1986690656 +73 06 39.284964108   12.006 11.927 11.712   ~ 525 0
13 V* AT Cnc CV* 08 28 36.9270732360 +25 20 03.045311628   14.798 14.583 13.690   DAe: 112 0
14 V* T Pyx CV* 09 04 41.5061511720 -32 22 47.502932700           ~ 440 0
15 V* BK Lyn CV* 09 20 11.2020621696 +33 56 42.356468364   13.97 13.99 14.72   ~ 118 1
16 NSV 18468 No* 10 38 22.51 -63 08 29.4           ~ 9 0
17 V* V382 Vel No* 10 44 48.3975221712 -52 25 31.168268472   15.945 15.737 16.173   ~ 192 0
18 V* CN Vel No* 11 02 38.6573695512 -54 23 09.487698612       16.5   ~ 25 1
19 WRAY 16-84 No* 11 03 15.8734539216 -58 27 26.066235276           ~ 30 1
20 V* V382 Cen EB* 11 33 54.5461006488 -60 50 32.097438672           ~ 4 0
21 LAWD 37 WD* 11 45 42.9169346379 -64 50 29.461957832 11.08 11.725 11.513 11.34 11.163 DQ 267 0
22 V* GQ Mus No* 11 52 02.4296561952 -67 12 20.986391520           ~ 264 0
23 NOVA Cru 1996 CV* 12 10 31.3654140720 -61 45 09.851097688           ~ 36 0
24 V* V888 Cen No* 13 02 31.8127250040 -60 11 36.147831720           ~ 33 0
25 V* V868 Cen No* 13 50 10.6971820608 -63 08 51.911816424           ~ 50 0
26 V* V842 Cen No* 14 35 52.5683885352 -57 37 35.391092232           ~ 146 0
27 V* BY Cir CV* 14 44 53.4742690968 -63 53 55.903194780           ~ 42 0
28 V* X Ser No* 16 19 17.6857680120 -02 29 29.533236000           ~ 69 0
29 V* U Sco CV* 16 22 30.7791646104 -17 52 43.166822628           F8+K2 549 0
30 V* OY Ara No* 16 40 50.4133579132 -52 25 50.699443507           ~ 38 0
31 V* V2109 Oph CV* 17 24 15.93 -24 36 50.2           ~ 19 0
32 V* V2104 Oph No* 18 03 24.9903588048 +11 47 57.063731712           ~ 23 0
33 V* V630 Sgr No* 18 08 48.3972106566 -34 20 21.660054088           ~ 46 0
34 V* V603 Aql No* 18 48 54.6369872232 +00 35 02.857106184 10.73 12.106 12.087 11.986   OB+e: 547 0
35 V* V604 Aql No* 19 02 06.33 -04 26 43.2           ~ 34 0
36 V* V1974 Cyg No* 20 30 31.6546001712 +52 37 50.837478240           ~ 579 0

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