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Dátum: 2010-08-28 09:03:01
Feladó: Gábor Sánta
Tárgy: Re: Fwd: AAVSO Special Notice #216: Two new FU Orionis variablesin Cygnus
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Ezek akkor most produk=C3=A1ltak FUOR kit=C3=B6r=C3=A9st?

=C3=89rdemes lenne keresni k=C3=B6r=C3=BCl=C3=B6tt=C3=BCk az =C3=BAjonnan m=
egjelen=C5=91 reeflexi=C3=B3s k=C3=B6d=C3=B6t, mint
a McNeil objektum eset=C3=A9ben.

Ott is a FUOR kit=C3=B6r=C3=A9s vil=C3=A1g=C3=ADtotta meg a port.

snt

2010/8/27 Bartha Lajos

>  K=C3=B6sz. Tartok t=C5=91le, hogy ezek kimaradnak a programomb=C3=B3l! B=
Q.
>
> ----- Original Message -----
> *From:* Kovi
> *To:* MIRA lista
> *Sent:* Friday, August 27, 2010 7:34 PM
> *Subject:* [Mira] Fwd: AAVSO Special Notice #216: Two new FU Orionis
> variablesin Cygnus
>
> M=C3=A9g alig csillagok, =C3=A9s m=C3=A1r v=C3=A1ltoz=C3=B3k! K=C3=A9t =
=C3=BAj objektum a Cygben, el=C3=A9gg=C3=A9
> halv=C3=A1nyak.
>
> Kvi
>
> -------- Original Message --------  Subject: AAVSO Special Notice #216:
> Two new FU Orionis variables in Cygnus Date: Fri, 27 Aug 2010 10:10:52
> -0400 From: aavso@aavso.org To: kovihome@freemail.hu
>
> AAVSO Special Notice #216
>
> Two new FU Orionis variables in Cygnus
> August 27, 2010
>
> Two new eruptive, pre-main sequence stars of FU Orionis type have
> recently been discovered in Cygnus.  Observations of both are encouraged
> to better characterize the behaviors of these two objects.
>
> The first object was an outburst of the star HBC 722 reported by E.
> Semkov and S. Peneva (Inst. of Astronomy, Sofia, Bulgaria) in ATel #2801
> (2010 Aug 17).  The object was reported to have risen by R=3D3.3
> magnitudes over the time span of 2010 May 13 to 2010 August 16.
> Subsequent spectroscopy reported by U. Munari et al. (ATel #2808, 2010
> Aug 23) support this object´s classification as an FU Orionis ("FU")
> star.  Munari et al. reported the object at V=3D14.04 on 2010 Aug 21.9.
>
> The second object was a new optical source discovered by K. Itagaki
> (Yamagata, Japan) on 2010 Aug 23.745 (JD 2455432.245) and reported in
> CBET 2426 (D.W.E. Green, editor).  As noted by H. Yamaoka in CBET 2426,
> the object appears faintly near magnitude 20 on a DSS image taken on
> 1990 Sep 11, but not on other plates.  The confirming optical image
> (CBET 2426) reported the object at an unfiltered magnitude of "about
> 13.8".  Subsequent spectroscopy and photometry of this object by U.
> Munari (CBET 2428) showed that this object also has the characteristics
> of an FU Ori star.  Munari reported the object at V=3D14.91 on 2010 Aug
> 26.83.
>
> The first object has the name "HBC 722" in AAVSO VSX.  It is located at
> the following (J2000) coordinates:
>
>         RA: 20 58 17.03 , Dec: +43 53 43.4
>
>
> The second object has been assigned the name "VSX J205126.1+440523" in
> AAVSO VSX.  It is located at the following (J2000) coordinates:
>
>         RA: 20 51 26.19 , Dec: +44 05 23.6
>
>
> Neither object currently has assigned comparison stars, so please
> clearly indicate your comparison and check stars when submitting data.
>
>
> Please use the names "HBC 722" and "VSX J205126.1+440523" when
> submitting data to the AAVSO.
>
>
> This AAVSO Special Notice was prepared by Matthew Templeton.
>
> ---------------------------------------------------
> SUBMIT OBSERVATIONS TO THE AAVSO
>
> Information on submitting observations to the AAVSO may be found at:http:=
//www.aavso.org/observing/submit/
>
> SPECIAL NOTICE ARCHIVE AND SUBSCRIPTION INFORMATION
>
> A Special Notice archive is available at the following URL:http://www.aav=
so.org/publications/specialnotice/
>
> Subscribing and Unsubscribing may be done at the following URL:http://www=
.aavso.org/publications/email/
>
>  ------------------------------
>
> ________________________________________________________________________
> Mira levelez=C5=91lista - V=C3=A1ltoz=C3=B3csillag-=C3=A9szlel=C5=91k f=
=C3=B3ruma
> Hozz=C3=A1sz=C3=B3l=C3=A1sok: Mira@mcse.hu
> Listakezel=C5=91 utas=C3=ADt=C3=A1sok: Mira-request@mcse.hu
> Arch=C3=ADvum, be=C3=A1ll=C3=ADt=C3=A1sok: http://mailman.mcse.hu/mailman=
/listinfo/mira
>
>
> ________________________________________________________________________
> Mira levelez=C5=91lista - V=C3=A1ltoz=C3=B3csillag-=C3=A9szlel=C5=91k f=
=C3=B3ruma
> Hozz=C3=A1sz=C3=B3l=C3=A1sok: Mira@mcse.hu
> Listakezel=C5=91 utas=C3=ADt=C3=A1sok: Mira-request@mcse.hu
> Arch=C3=ADvum, be=C3=A1ll=C3=ADt=C3=A1sok: http://mailman.mcse.hu/mailman=
/listinfo/mira
>

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Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

Ezek akkor most produk=C3=A1ltak FUOR kit=C3=B6r=C3=A9st?

=C3=89rdem=
es lenne keresni k=C3=B6r=C3=BCl=C3=B6tt=C3=BCk az =C3=BAjonnan megjelen=C5=
=91 reeflexi=C3=B3s k=C3=B6d=C3=B6t, mint a McNeil objektum eset=C3=A9ben. =


Ott is a FUOR kit=C3=B6r=C3=A9s vil=C3=A1g=C3=ADtotta meg a port. r>
snt


2010/8/27 Bartha Lajos <=
;arbar@t-online.hu>

<=
blockquote class=3D"gmail_quote" style=3D"border-left: 1px solid rgb(204, 2=
04, 204); margin: 0pt 0pt 0pt 0.8ex; padding-left: 1ex;">







K=C3=B6sz. Tartok t=C5=91le, hogy ezek=
kimaradnak a=20
programomb=C3=B3l! BQ.

x; padding-left: 5px; margin-left: 5px; margin-right: 0px;">
>

 
l; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adj=
ust: none; font-stretch: normal;">----- Original Message -----

 
oz-background-clip: -moz-initial; -moz-background-origin: -moz-initial; -mo=
z-background-inline-policy: -moz-initial; font-family: arial; font-style: n=
ormal; font-variant: normal; font-weight: normal; font-size: 10pt; line-hei=
ght: normal; font-size-adjust: none; font-stretch: normal;">
From:=20
  rget=3D"_blank">Kovi=20
 

 
l; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adj=
ust: none; font-stretch: normal;">To: =3D"mailto:mira@mcse.hu" target=3D"_blank">MIRA lista


 
l; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adj=
ust: none; font-stretch: normal;">Sent: Friday, August 27, 2010 7:34=
=20
  PM

 
l; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adj=
ust: none; font-stretch: normal;">Subject: [Mira] Fwd: AAVSO Special=
Notice=20
  #216: Two new FU Orionis variablesin Cygnus

 

M=C3=A9g alig csillagok, =C3=A9s m=C3=A1r v=C3=A1ltoz=C3=
=B3k! K=C3=A9t =C3=BAj objektum a Cygben,=20
  el=C3=A9gg=C3=A9 halv=C3=A1nyak.

Kvi

-------- Original Mess=
age --------=20
 
   
   
     
     
   
     
     
   
     
     
   
     
     
Subject: AAVSO Special Notice #216: Two new FU Orionis variables in=20
    Cygnus
Date: Fri, 27 Aug 2010 10:10:52 -0400
From: aavso@aavso.=
org
To: kovihom=
e@freemail.hu


AAVSO Special Notic=
e #216

Two new FU Orionis variables in Cygnus
August 27, 2010

Two new eruptive, pre-main sequence stars of FU Orionis type have
recently been discovered in Cygnus.  Observations of both are encouraged
to better characterize the behaviors of these two objects.

The first object was an outburst of the star HBC 722 reported by E.
Semkov and S. Peneva (Inst. of Astronomy, Sofia, Bulgaria) in ATel #2801
(2010 Aug 17).  The object was reported to have risen by R=3D3.3
magnitudes over the time span of 2010 May 13 to 2010 August 16.=20
Subsequent spectroscopy reported by U. Munari et al. (ATel #2808, 2010
Aug 23) support this object's classification as an FU Orionis ("FU=
")
star.  Munari et al. reported the object at V=3D14.04 on 2010 Aug 21.9.

The second object was a new optical source discovered by K. Itagaki
(Yamagata, Japan) on 2010 Aug 23.745 (JD 2455432.245) and reported in
CBET 2426 (D.W.E. Green, editor).  As noted by H. Yamaoka in CBET 2426,
the object appears faintly near magnitude 20 on a DSS image taken on
1990 Sep 11, but not on other plates.  The confirming optical image
(CBET 2426) reported the object at an unfiltered magnitude of "about
13.8".  Subsequent spectroscopy and photometry of this object by U.
Munari (CBET 2428) showed that this object also has the characteristics
of an FU Ori star.  Munari reported the object at V=3D14.91 on 2010 Aug
26.83.

The first object has the name "HBC 722" in AAVSO VSX.  It is loca=
ted at
the following (J2000) coordinates:

        RA: 20 58 17.03 , Dec: +43 53 43.4


The second object has been assigned the name "VSX J205126.1+440523&quo=
t; in
AAVSO VSX.  It is located at the following (J2000) coordinates:

        RA: 20 51 26.19 , Dec: +44 05 23.6


Neither object currently has assigned comparison stars, so please
clearly indicate your comparison and check stars when submitting data.


Please use the names "HBC 722" and "VSX J205126.1+440523&quo=
t; when
submitting data to the AAVSO.


This AAVSO Special Notice was prepared by Matthew Templeton.

---------------------------------------------------
SUBMIT OBSERVATIONS TO THE AAVSO

Information on submitting observations to the AAVSO may be found at:
http:/=
/www.aavso.org/observing/submit/


SPECIAL NOTICE ARCHIVE AND SUBSCRIPTION INFORMATION

A Special Notice archive is available at the following URL:
nk">http://www.aavso.org/publications/specialnotice/

Subscribing and Unsubscribing may be done at the following URL:
http=
://www.aavso.org/publications/email/



 


 




 

__________________________________________________________________=
______
Mira=20
  levelez=C5=91lista - V=C3=A1ltoz=C3=B3csillag-=C3=A9szlel=C5=91k f=C3=B3r=
uma
Hozz=C3=A1sz=C3=B3l=C3=A1sok:=20
  Mira@mcse.hu
Lis=
takezel=C5=91 utas=C3=ADt=C3=A1sok: target=3D"_blank">Mira-request@mcse.hu
Arch=C3=ADvum,=20
  be=C3=A1ll=C3=ADt=C3=A1sok:=20
=
http://mailman.mcse.hu/mailman/listinfo/mira


_______________________________________________________________________=
_

Mira levelez=C5=91lista - V=C3=A1ltoz=C3=B3csillag-=C3=A9szlel=C5=91k f=C3=
=B3ruma

Hozz=C3=A1sz=C3=B3l=C3=A1sok: Mira@mcse.hu<=
/a>

Listakezel=C5=91 utas=C3=ADt=C3=A1sok:
hu">Mira-request@mcse.hu

Arch=C3=ADvum, be=C3=A1ll=C3=ADt=C3=A1sok: u/mailman/listinfo/mira" target=3D"_blank">http://mailman.mcse.hu/mailman/l=
istinfo/mira




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