2010IAUC.9167....3Y

Query : 2010IAUC.9167....3Y

2010IAUC.9167....3Y - IAU Circ., 9167, 3 (2010/September-0)

Nova Aquilae 2010.

YAMANAKA M., ITOH R. and KOMATSU T.

Abstract (from CDS):

M. Yamanaka, R. Itoh, and T. Komatsu, Hiroshima University, report that they obtained a low-resolution optical spectrum (range 450-900 nm; R = 400) of the nova on Sept. 11.60 UT at the Higashi- Hiroshima Observatory of Hiroshima University. The spectrum shows a highly reddened continuum and no strong emission line below 600 nm. The H_alpha feature, whose emission line full-width-at-zero- intensity (FWZI) is measured to be 3000 km/s, has a P-Cyg profile; the H_alpha absorption component has FWZI = 1500 km/s. An H_beta feature is not detected in the spectrum. O I 777.4-nm and O I 844.6-nm also exhibit P-Cyg line profiles, and their absorption minima reach 1500 km/s. The Ca II near-infrared triplet lines 849.8-, 854.2-, and 866.2-nm exhibit strong emission. The absorption of Ca II 866.2-nm has FWZI = 1500 km/s. The Paschen line series is also confirmed. These characteristics suggest that this nova is a "Fe II"-type nova.

Abstract Copyright: ∼

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Status at CDS : Objects in title, abstract, text, figures, and all or part of small table(s) being processed in SIMBAD.

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* V1723 Aql No* 18 47 38.38 -03 47 14.1           ~ 31 0

Query : 2010IAUC.9167....3Y

Basic data :
V* V1723 Aql -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA), V* (V*)
ICRS coord. (ep=J2000) : 		18 47 38.38 -03 47 14.1 [ ] D ~
FK4 coord. (ep=B1950 eq=1950) : 		18 45 00.23 -03 50 35.3 [ ]
Gal coord. (ep=J2000) : 		029.12851 -00.88249 [ ]
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Identifiers (2) :
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NOVA Aql 2010 V* V1723 Aql

References (31 between 1850 and 2026) (Total 31)
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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Distance : 1   

   

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V* V1723 Aql

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