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[vsnet-alert 840] V1413 Aql (=AS 338)
- Date: Fri, 11 Apr 1997 16:40:30 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 840] V1413 Aql (=AS 338)
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
The eclipsing symbiotic nova V1413 Aql = AS 338 is undergoing a sudden
drop in magnitude as indicated by the following observations.
YYMMDD(UT) mag code
970301.205 121 POY
970320.160 122 POY
970327.106 122 POY
970329.105 122 POY
970401.167 123 POY
970410.133 138 POY
The outburst and eclipsing nature of this object was discovered by
M. Wakuda (VSOLJ Variable Star Bulletin 5, 17, 1988), who gave the following
eclipse ephemeris:
Min = JD 2445784 + 434 E
The system was further studied by U. Munari (Astron. Astrophys. 257,
163, 1992) who gave an improved ephemeris:
Min = JD 2446650 + 434.1 E
+/-15 +/-0.2
Munari concluded from optical and UV spectroscopy and photometry that
the object, composed by an M5 III star and a very hot compact star,
presumably resulting a symbiotic nova-type thermonuclear runaway (TNR)
without a detectable mass ejection. Observations during the present
eclipse are highly encouraged since the object is currently experiencing
strong multiple reflares starting in 1992 (the largest one in 1995).
Reported observations show a considerable scatter. The V-band VSNET
chart dated 1996 Sep. 9 would solve the problem in comparison stars.
Regards,
Taichi Kato
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