Sziasztok!

Az orosz MASTER csapat egy ujabb, fenyes torpe novat talalt, ezuttal az
Aurigaban:

MASTER OT J064725.70+491543.9

Csutortok hajnalban 13,2 magni korul volt a fenyessege. A VSNET-en jott
hirek szerint szuperpupokat is eszleltek a csillagnal, szoval ugy nez
ki, SU UMa tipusu.

A hirek szerint 2003. januarjaban a Palomar/NEAT, 2007. oktobereben a
CRTS felveteleink latszik kitoresben a csillag. 2012. augusztus 20-an a
MASTER-Amur felvetelen megfigyelheto 13,9 magnitudo fenyessegnel, de csak
egy kepen latszik, s viszont egy kitores detektalasahoz ket kepen kell
latszania egy objektumnak, emiatt nem vettek eszre akkor.

A csillaghoz keszult friss, ropogos AAVSO oh-sorozat, a terkepe
letolheto a VSP-rol.

Hetfo este lefotoztam a teruletet, hamarosan megnezem, hogy latszik-e
meg a kepeimen az ujonnan felfedezett fenyes torpe nova.

* * *

Mas:
- a hirek szerint kitor a QW Ser torpe nova is. Hajnali egen erdemes
megprobalkozni vele.

udv:

Fidusz

* * *

From: Denis Denisenko
Date: 2013/3/8
Subject: [vsnet-alert 15474] New bright CV in Auriga MASTER OT
J064725.70+491543.9 (13.2m)


Pavel Balanutsa has found a very bright optical transient on 2013 Mar.
07 MASTER-Amur survey images. The discovery was reported in ATel
#4871, see .

MASTER OT J064725.70+491543.9
  20130307.710  133C  MASTER-Amur
  20130307.712  132C  MASTER-Amur

This is the 5th brightest dwarf nova among more than 110 CVs
discovered by MASTER so far.

The object has quiescent counterparts in several catalogs:
USNO-A2.0 1350-06816147  06 47 25.82 +49 15 43.3  R=17.5  B=17.5
USNO-B1.0 1392-0177998  06 47 25.697 +49 15 42.76
pmRA=-24 pmDE=-14 B1=17.92 R1=17.16 B2=17.07 R2=17.17 I=16.83
GALEX J064725.6+491542 FUV=18.32+/-0.05 NUV=18.25+/-0.03
1RXS J064725.3+491539 0.032+/-0.012 cnts/s HR1=1.00+/-0.41 HR2=0.69+/-0.25

Previous outbursts were observed by Palomar/NEAT on 2003 Jan. 08-10
and by Catalina Sky Survey on 2007 Oct. 10 (14.1m). MASTER-Amur had
also observed the star in outburst on 2012 Aug. 20.756 UT (13.9m), but
on a single image only, and that outburst was missed (two detections
are required for a real transient). Star was also bright on 1993 Dec.
10 blue POSS-II plate (USNO-B value of B2=17.07 was measured from the
1990 Feb. 15 plate at quiescence).

The object may be a new UGSU variable. Photometric time series are encouraged!

Discovery and reference images:
http://master.sai.msu.ru/static/OT/064725.70491543.8.png

Denis Denisenko
Member of MASTER team at SAI MSU

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