[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-campaign-news 174] Bright (5-6 mag) likely nova in Sgr




  ====================================================================
            Bright (5-6 mag) likely nova in Sagittarius
  ====================================================================

  Katsumi Haseda (Aichi Japan) has discovered a bright new object (most likely
a nova) in Sagittarius.  The details are as follows:

[All messages are from vsnet-discovery-nova messages.]

Unconfirmed bright object(?) in Sgr, please confirm!

    Katsumi Haseda (Aichi Japan) has reported possible detection of
a potentially bright object (mag about 5.0) at an approximate position
190108.5 -220045 (J2000.0).  Since the stellar image was recorded
on a single film taken on 2002 Sep. 20.431 UT, the existence or reality of
the object has not been confirmed.  Although we don't usually report
a potential discovery alert at such an early stage, I relay this report
because the exceptional brightness clearly requires emergent confirmation.

    Could someone check this field?

---

New object confirmed at position 19 01 09.34 -22 00 05.5 at 09/21/2002 1:35 
UT.  Position based on plate solution with 20 GSC 1.1 stars.  V magnitude 
greater than 6.3 based on magnitudes in TheSky software.  My 20 second 
exposure was in saturation.  I compared two V band images to DSS1.V.SERC V 
band epoch 1987.59 image.  The new object is stellar in appearance and is not 
present on the DSS1 image.  I will continue with photometry and 
spectrophotometry and report observations when they are reduced.

Regards,
Doug West

---

I confirmed visually, mag. 6.1 on Sep 21.145 at position 19 01 09 (+/-
1s) -22 00 05 (+/- 5")
using  80 mm refractor f/5 with setting circles. Comp stars SAO 185584 &
187519 & 187422.
Regards
Jaime Garcia (GAJ)
Argentina

---

Additional photometry of the object at 19 01 09.38 -22 00 05.9 error +/- 
0.75".  This position was measured from a 5 second exposure image.  The plate 
solution used 20 GSC 1.1 stars.  B=6.44 +/-0.6, V<6.0 (the 5 second exposure 
was in saturation).  Comparison stars:  SAO 187580 B=10.34 V=9.21 and SAO 
187591 B=8.98 V=8.75.   The images were taken under clear skies with a full 
moon.  I will reduce the low-resolution spectroscopy in the morning and post 
it on my web page.

Regards,
Doug West
Mulvane, KS USA
http://hometown.aol.com/dwest61506/index.html

---

Regards,
Taichi Kato
VSNET Collaboration team

----------------------------------------------------------------------------

  VSNET (Variable Star Network) is an international variable star observing
network, covering various areas of novae, supernovae, cataclysmic variables
(CVs), X-ray transients, and other classical eruptive, pulsating, and
eclipsing variables.  VSNET is one of invited contributing organizations
to the SkyPub AstroAlert system.

       VSNET Home Page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/

CCD observations of such targets are a relatively easy task for a 20-40cm
telescope; simply take as many CCD frames (with exposure times 10-30 sec)
as possible, spanning several hours per night.  The only requirements are
the weather and your patience!  If you need more help on the observing
technique, please feel free to ask on the vsnet-campaign list.

   We would sincerely appreciate volunteers who would join the VSNET
Collaboration team to study the wonders of these exotic variable stars.
To join the VSNET campaign collaborative list, send an e-mail to

         vsnet-adm@kusastro.kyoto-u.ac.jp (VSNET administrator)

with a line "SUBSCRIBE vsnet-campaign." or your comment to join the
collaboration team.

----------------------------------------------------------------------------

VSNET Home Page

Return to Daisaku Nogami


vsnet-adm@kusastro.kyoto-u.ac.jp