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G=E1bor, k=E9t tranziens is van egy id=F5ben, az egyik egy Mira val=F3j=E1b=
an, a
m=E1sik minden jel szerint t=F6rpen=F3va. Ut=F3bbir=F3l egy r=F6vid besz=E1=
mol=F3t m=E9g az
=E9jjel bek=FCldt=FCnk a CBET-nek, fyi idem=E1solom:
PNV J17522579-2126215
L. Kiss, K. S=E1rneczky (Konkoly Observatory, Hungary), J. Kov=E1cs and T.
Borkovits (ELTE Gothard Observatory, Hungary) report on
a medium-resolution optical spectrogram obtained with the 0.5m RC telescope
of the Gothard Observatory on 2012 June 26.95 UT.
The spectrum does not contain any strong emission lines, with clearly
identifiable H-beta line in absorption and a strong interstellar absorption
of the sodium D doublet. The H-alpha line is possibly seen in absorption.
Two narrow emission lines are also visible around 5750 A, each with an FWZI
about 60 km/s. The spectrum safely excludes the nova nature of the object,
which is presumably a dwarf nova in outburst phase. The estimated visual
brightness of the target was about 9.5 mag, based on the guider image.
Ksl
2012/6/27 G=E1bor S=E1nta
> Most akkor mira vagy UGWZ vagy N???
>
> snt
>
> FIDRICH Robert =EDrta, 2012.06.27.:
> > Nanu!
> >
> >> A fene ebbe a sok n=F3v=E1ba a Sgr-ben. =C9n err=F5l =EDrtam, amit =ED=
rtam:
> >> PNV J17522579-2126215 2012 06 26.5494* 17 52 25.79 -21 26 21.5 10.3=
U
> >
> > Hm, errol meg en nem hallottam meg. Ahogy latom, ez is friss felfedezes=
,
> > es viszonylag eszakon van ez is.
> >
> > Torpenovanak nem tul fenyes? Vagy UGWZ tipusu? A szinkepet bekuldtetek
> > mar az IAU-nak?
> >
> >
> >> A Fidusz =E1ltal eml=EDtett PNV J18351050-1919300 egy ismert mira t=ED=
pus=FA
> >> v=E1ltoz=F3 (ASAS 183511-1919.5 =3D 2MASS 18351047-1919298)
> >
> > Amikor en neztem, ez meg nem szerepelt a CBET honlapon. Latom, azota ma=
r
> > mas is irta, hogy mira.
> >
> > udv:
> >
> > --
> > Fidusz (FIDRICH Robert)
> > drotlevel:fidusz@zpok.hu
> > #jabber/gtalk: fidusz@jabber.hu
> > _______________________________________________________________________=
_
> > Mira levelez=F5lista - V=E1ltoz=F3csillag-=E9szlel=F5k f=F3ruma
> > Hozz=E1sz=F3l=E1sok: Mira@mcse.hu
> > Listakezel=F5 utas=EDt=E1sok: Mira-request@mcse.hu
> > Arch=EDvum, be=E1ll=EDt=E1sok: http://mailman.mcse.hu/mailman/listinfo/=
mira
> >
> ________________________________________________________________________
> Mira levelez=F5lista - V=E1ltoz=F3csillag-=E9szlel=F5k f=F3ruma
> Hozz=E1sz=F3l=E1sok: Mira@mcse.hu
> Listakezel=F5 utas=EDt=E1sok: Mira-request@mcse.hu
> Arch=EDvum, be=E1ll=EDt=E1sok: http://mailman.mcse.hu/mailman/listinfo/mi=
ra
>
--=20
L=E1szl=F3 L. Kiss
Scientific advisor & Lend=FClet project leader
Konkoly Observatory
Hungarian Academy of Sciences
klaci72@skype
Web: http://www.konkoly.hu/staff/kiss
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G=E1bor, k=E9t tranziens is van egy id=F5ben, az egyik egy Mira val=F3j=E1b=
an, a m=E1sik minden jel szerint=A0t=F6rpen=F3va. Ut=F3bbir=F3l egy r=F6vid=
besz=E1mol=F3t m=E9g az =E9jjel bek=FCldt=FCnk a CBET-nek, fyi idem=E1solo=
m:
PNV J17522579-2126215
L. Kiss, K. S=E1rneczky (Konkoly Observatory, Hungary), J. Kov=E1cs and=
T. Borkovits (ELTE Gothard Observatory, Hungary) report =A0on=A0
a medi=
um-resolution optical spectrogram obtained with the 0.5m RC telescope of th=
e Gothard Observatory on 2012 June 26.95 UT.
The spectrum does not contain any strong emission lines, with clearly ident=
ifiable H-beta line in absorption and a strong interstellar absorption of t=
he sodium D doublet. The H-alpha line is possibly seen in absorption. Two n=
arrow emission lines are also visible around 5750 A, each with an FWZI abou=
t 60 km/s. The spectrum safely excludes the nova nature of the object, whic=
h is presumably a dwarf nova in outburst phase. The estimated visual bright=
ness of the target was about 9.5 mag, based on the guider image.
Ksl
2012/6/27 G=E1bor S=E1=
nta
<
=3D"_blank">saga21enator@gmail.com>
mail_quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-l=
eft:1ex">
Most akkor mira vagy UGWZ vagy N???
snt
FIDRICH Robert <fidusz@zpok.hu>=
=EDrta, 2012.06.27.:
--
=
arial,sans-serif;font-size:13px">L=E1szl=F3 L. KissScientific advisor &a=
mp;=A0
204);color:rgb(34,34,34);background-repeat:initial initial">Lend=FClet
n>=A0project=A0
(255,255,204);color:rgb(34,34,34);background-repeat:initial initial">leader=
Konkoly Observatory
Hungarian Academy of Sciences
klaci72@skype
We=
b:=A0
204)" target=3D"_blank">http://www.konkoly.hu/staff/kiss
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