2024RNAAS...8..317R

Query : 2024RNAAS...8..317R

2024RNAAS...8..317R - Research Notes of the AAS, 8, 317 (2024/December-0)

V1663 Aquilae: A Fast Fe II-type Nova that Formed Dust and Coronal Lines.

RUDY R.J., RUSSELL R.W., LYNCH D.K. and PUETTER R.C.

Abstract (from CDS):

V1663 Aquilae was a rare nova that formed both dust and coronal emission lines. A spectrum from 157 days after peak brightness shows both thermal dust emission and coronal emission present at the same epoch. An earlier spectrum from 36 days post maximum captures the nova prior to the formation of either dust or high-excitation emission lines. At the earlier epoch, its emission lines arose mostly from neutral species and singly ionized iron.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Classical novae - Novae - Classical novae - Novae

Simbad objects: 2

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Number of rows : 2
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 HD 168646 * 18 22 00.1406039376 -28 25 47.875197468   6.396 6.154     A3III 38 0
2 V* V1663 Aql No* 19 05 12.50 +05 14 12.0           Kep 39 0

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