2009CBET.2075....1N


Query : 2009CBET.2075....1N

2009CBET.2075....1N - Central Bureau Electronic Telegrams, 2075, 1 (2009/December-0)

Nova Aquilae 2009.

NISHIYAMA K., KABASHIMA F., CORELLI P. and VOLLMANN W.

Abstract (from CDS):

Koichi Nishiyama, Kurume, Fukuoka-ken, Japan; and Fujio Kabashima, Miyaki-cho, Saga-ken, Japan, report their discovery of a possible nova (mag 10.9) on two 40-s unfiltered CCD frames (limiting magnitude 13.3) taken on Dec. 14.398 and 14.399 UT using a 105-mm f/4 camera lens. Seven confirming unfiltered CCD frames (limiting magnitude 18.4) taken around Dec. 14.408 using a 0.40-m f/9.8 reflector yield mag 10.9 and the following position for the new star: R.A. = 19:14:09.73, Decl. = +15:16:34.7 (equinox 2000.0). Nothing is visible at this position on their two survey frames taken on Dec. 6.417 (limiting mag 13.7) and 7.412 (limiting mag 13.6). Following posting on the CBAT unconfirmed-objects webpage, P. Corelli (Pagnacco, Italy, 0.45-m f/4.4 reflector) writes that his 5-s unfiltered CCD exposure taken on Dec. 14.791 yields mag 10.8 and position end figures 09s.69, 34".0; Corelli adds that nothing is visible at this position on a Digitized Sky Survey plate (limiting red mag approximately 21.5). Visual magnitude estimate for the variable by W. Vollmann, Vienna, Austria: Dec. 14.710, 11.4.

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* V1722 Aql No* 19 14 09.73 +15 16 34.7           ~ 19 0

Query : 2009CBET.2075....1N

Basic data :
V* V1722 Aql -- Classical Nova
Other object types:
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No* (2017ARep,NOVA), V* (V*)
ICRS coord. (ep=J2000) :
19 14 09.73 +15 16 34.7 [ ] D 2009IAUC.9100....1N
FK4 coord. (ep=B1950 eq=1950) :
19 11 53.23 +15 11 20.7 [ ]
Gal coord. (ep=J2000) :
049.08498 +02.01448 [ ]
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Identifiers (2) :
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NOVA Aql 2009 V* V1722 Aql

References (19 between 1850 and 2026) (Total 19)
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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V* V1722 Aql

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