SETI public: Possible Nova Near the Small Magellanic Cloud

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From: LARRY KLAES (ljk4@msn.com)
Date: Thu Oct 17 2002 - 21:52:55 PDT


----- Original Message -----
From: aavso@aavso.org
Sent: Thursday, October 17, 2002 5:18 PM
To: aavso@aavso.org
Subject: AAVSO News Flash #1046

              THE AMERICAN ASSOCIATION OF VARIABLE STAR OBSERVERS
                   25 Birch Street, Cambridge, MA 02138 USA
                   Tel. 617-354-0484 Fax 617-354-0665
                            http://www.aavso.org

                        * * * AAVSO NEWS FLASH * * *

Subject: 0053-73 N SMC 02 No. 1046
         HST Observations October 17, 2002
         1848+26 CY LYR
----------------------------------------------------------------------------
0053-73 POSSIBLE NOVA IN THE SMALL MAGELLANIC CLOUD

We have been informed by the Central Bureau for Astronomical Telegrams
(IAU Circular 7995) that a possible nova near the center of the Small
Magellanic Cloud has been discovered by W. Liller of Chile. The 12.3
magnitude object appears on Technical Pan exposures taken on OCT 16.2 UT.

A CCD exposure taken by Liller at OCT 17.204 UT was used to obtain a
broadband V magnitude of 12.66 and the following position:

  R.A.= 0h 56m 30.4s +/- 0.2s Decl.= -72o 36' 29.4" +/- 1.1" (2000)

Please report the object to the AAVSO as: 0053-73 N SMC 02

An AAVSO chart prepared by Aaron Price and showing the location of the
possible nova has been posted on the AAVSO web page. This chart is
accessible via the following url: http://charts.aavso.org/

Congratulations to W. Liller on this discovery!
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HST TO OBSERVE CW1045+525, V503 CYG, AND BZ UMA

We have been informed by one of our colleagues that the Space Telescope
Imaging Spectrograph aboard the Hubble Space Telescope will be doing
ultraviolet spectroscopy of CW1045+525, V503 Cyg, and BZ UMa in the
coming week. The exact times of the scheduled observations are given
below:

CW1045+525 Oct 18 2002 08:56:24 UT to 09:42:47 UT
V503 Cyg Oct 24 2002 15:46:35 UT to 16:22:54 UT
BZ UMa Oct 25 2002 04:17:39 UT to 04:56:39 UT

Observers, especially those with CCDs, are encouraged to keep a close
eye on these objects leading up to and particularly during the HST
observations. Having AAVSO data available for correlation will be
very useful to our colleagues in the analysis of their HST data.
----------------------------------------------------------------------------
1848+26 CY LYRAE

The dwarf nova type cataclysmic variable CY LYR appears to be in outburst,
as indicated by the following observations:

                     AAVSO Observer AAVSO Observer
    UT Mag. Initials UT Mag. Initials

OCT 15.0194 15.99 CCDV GKA OCT 15.0410 <14.0 TSC
OCT 15.0278 <14.8 TDB OCT 17.0972 13.7 TDB
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We thank the following contributors for the data that they
have provided for this News Flash:

GKA - K. GRAHAM, USA TSC - S. TRACY, USA
TDB - D. TAYLOR, CANADA

Please monitor these and other variable stars closely and phone-in, fax,
or e-mail your observations to the AAVSO.

Good observing!
Janet A. Mattei, Director
Rebecca Pellock, Technical Assistant
____________________________________________________________________________
Symbols may include: < = fainter than magnitude given (variable not seen)
                      : = uncertain
                   CCDV = Charge-coupled device with (V) filter

If you would like to contribute to AAVSO NEWS FLASH, please send
observations of unusual variable star activity to:

                     observations@aavso.org

Those who wish to subscribe (free of charge) or unsubscribe to NEWS FLASH
may do so by visiting the following web page:

                      http://www.aavso.org

If you would like data from the AAVSO International Database for
research purposes, please send your request to:

        Janet Mattei, AAVSO Director, at aavso@aavso.org

An archive of past issues of the News Flash is available
at the following web page:

                      http://www.aavso.org/newsflash/

We look forward to including your observations in future editions
of AAVSO NEWS FLASH!
____________________________________________________________________________


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