2007IAUC.8896....2N


Query : 2007IAUC.8896....2N

2007IAUC.8896....2N - IAU Circ., 8896, 2 (2007/November-0)

V597 Puppis = Nova Puppis 2007.

NAITO H. and TOKIMASA N.

Abstract (from CDS):

H. Naito and N. Tokimasa, Nishi-Harima Astronomical Observatory, report that they obtained a low-resolution spectrum (range 410-670 nm; resolution 1200 at H_alpha) of V597 Pup on Nov. 14.77 UT with the 2.0-m NAYUTA telescope (+ MALLS). The spectrum shows broad Balmer lines and Fe II (42 multiplet) with P-Cyg features, as well as blueshifted absorption lines of Fe II (49, 74), O I 615.5-615.8 nm, and Si II 634.7-nm. The nova belongs to the Fe II type and was caught near maximum light. A narrow Na I D absorption line (EW = 0.3 nm) indicates that some interstellar reddening exists. The expansion velocities derived from the FWHM of the Balmer features H_alpha, H_beta, and H_gamma are 1800, 1700, and 1800 km/s, respectively.

Abstract Copyright: ∼

Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
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 V* V597 Pup No* 08 16 17.9596509204 -34 15 24.933440401   21.65       ~ 56 0

Query : 2007IAUC.8896....2N

Basic data :
V* V597 Pup -- Classical Nova
Other object types:
otypes_help
No* (2017ARep,NOVA), * (GSC2.3,Gaia), CV* (2020MNRAS), V* (V*)
ICRS coord. (ep=J2000) :
08 16 17.9596509204 -34 15 24.933440401 (Optical) [ 0.2862 0.3793 90 ] A 2018yCat.1345....0G
FK4 coord. (ep=B1950 eq=1950) :
08 14 21.9260768979 -34 06 07.058619755 [ 0.2862 0.3793 90 ]
Gal coord. (ep=J2000) :
252.5294627481079 +00.5453097339321 [ 0.2862 0.3793 90 ]
Proper motions mas/yr :
-2.282 3.783 [0.695 0.947 90] A 2018yCat.1345....0G
Parallaxes (mas):
0.0113 [0.4780] A 2018yCat.1345....0G
Fluxes (2) :
B 21.65 [0.48] E 2008AJ....136..735L
G 20.0173 [0.0158] C 2018yCat.1345....0G
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Identifiers (4) :
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NOVA Pup 2007 GSC2.3 S65B052556 V* V597 Pup Gaia DR2 5546402675939272576

References (56 between 1850 and 2026) (Total 56)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 1    Plx : 1    PM : 1   

   


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V* V597 Pup Gaia DR2 5546402675939272576

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