1998ApJ...506..818D

Query : 1998ApJ...506..818D

1998ApJ...506..818D - Astrophys. J., 506, 818-823 (1998/October-3)

The spectroscopic differences between disk and thick-disk/bulge novae.

DELLA VALLE M. and LIVIO M.

Abstract (from CDS):

We examine a sample of novae with distances that have been mostly determined by nebular parallaxes and determine their spectral classes according to the classification of Williams. We show that novae that have been classified as He/N tend to concentrate close to the Galactic plane and are fast and bright, while Fe II novae are slow and faint and are distributed more homogeneously up to heights of ∼1000 pc above the Galactic plane. We identify a quantitative characterization of the prototypical ``fast'' and ``slow'' novae.

Abstract Copyright: ∼

Journal keyword(s): Stars: Novae, Cataclysmic Variables - Stars: Evolution - Stars: White Dwarfs

Simbad objects: 30

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Number of rows : 30
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 M 33 GiG 01 33 50.8965749232 +30 39 36.630403128 6.17 6.27 5.72     ~ 6226 1
3 V* GK Per No* 03 31 12.0098863320 +43 54 15.469951212   14.139 13.090 12.589   K1IV 986 0
4 V* XX Tau No* 05 19 24.4641860376 +16 43 00.414603372           ~ 56 0
5 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
6 V* T Aur No* 05 31 59.1180488976 +30 26 45.034081044           ~ 291 0
7 V* RR Pic No* 06 35 36.0630266144 -62 38 24.291214934   12.407 12.449 12.675 12.385 ~ 368 0
8 V* V351 Pup No* 08 11 38.3931386664 -35 07 30.288675216           ~ 128 0
9 V* CP Pup No* 08 11 46.0634106720 -35 21 04.986480708   15.436 15.227     ~ 277 1
10 V* V868 Cen No* 13 50 10.6971820608 -63 08 51.911816424           ~ 51 0
11 V* RW UMi No* 16 47 54.8186248248 +77 02 12.047306028           ~ 79 0
12 V* V2264 Oph No* 17 20 20.83 -26 46 26.3           ~ 46 0
13 V* V745 Sco Sy* 17 55 22.2260994408 -33 14 58.551839808     17.987   13.353 M2/M6IIIe 265 1
14 V* DQ Her CV* 18 07 30.2510391864 +45 51 32.564791872   14.605 14.443 14.800   M3+Ve 1048 1
15 V* V533 Her No* 18 14 20.4844831200 +41 51 22.069747872   15.000 15.032 15.274   ~ 265 0
16 V* V3890 Sgr No* 18 30 43.2877623168 -24 01 08.944843980     15.944 14.798 12.611 M5III 232 0
17 V* FH Ser No* 18 30 47.0401403328 +02 36 52.029761940           ~ 215 0
18 V* V838 Her No* 18 46 31.4714863335 +12 14 02.104189516           ~ 304 0
19 V* V603 Aql No* 18 48 54.6369872232 +00 35 02.857106184 10.73 12.106 12.087 11.986   OB+e: 564 0
20 V* V446 Her No* 18 57 21.5916294048 +13 14 29.316793632           ~ 152 0
21 V* V1229 Aql No* 19 24 44.52 +04 14 48.7           ~ 63 0
22 V* LV Vul No* 19 48 00.43728 +27 10 17.3640           ~ 115 0
23 V* V500 Aql No* 19 52 27.9896199327 +08 28 46.958265972           ~ 45 0
24 V* V476 Cyg No* 19 58 24.5056065864 +53 37 06.921041340           ~ 121 0
25 V* QU Vul No* 20 26 46.0200167016 +27 50 43.163406959           ~ 277 0
26 V* V1974 Cyg No* 20 30 31.6546001712 +52 37 50.837478240           ~ 597 0
27 V* HR Del No* 20 42 20.3468874528 +19 09 39.305636208   12.380 12.404 12.508   ~ 515 0
28 V* V1500 Cyg No* 21 11 36.5809818696 +48 09 01.952490204           ~ 820 0
29 V* CP Lac No* 22 15 41.1032963832 +55 37 01.322162256           ~ 142 1
30 V* DK Lac No* 22 49 46.9311405048 +53 17 19.798203336           ~ 116 0

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