SUBJECTS:
1. POSSIBLE NOVA IN PYXIS: 0914-29 N PYX 05
2. NEW PROBABLE CATACLYSMIC VARIABLE: 0523+62 RXSJ053234 (BERNHARD01)
3. FOLLOW-UP ON REQUEST TO MONITOR U GEM
1. 0914-29 N PYX 05 - POSSIBLE NOVA
Event: Apparent nova
Discovered Independently By (IAU Circular 8495):
- the All Sky Automated Survey (ASAS) (65-mm-aperture telephoto lens) and
reported by G. Pojmanski, Warsaw University Astronomical Observatory;
- H. Haseda, Aichi, Japan, and reported by H. Yamaoka, Kyushu University,
Japan
Discovery Magnitude (IAU Circular 8495):
- 12.0 V (ASAS)
- 13.3 (0.10-m twin patrol camera) (Haseda)
Discovery Date (IAU Circular 8495):
- March 11.191 UT (ASAS)
- March 16.45 UT (Haseda)
Position: R.A. (2000): 09h 18m 58s Decl. (2000): -29o 42' 36" (ASAS)
Spectra: none
AAVSO Chart(s): No AAVSO chart has been made yet for this object. Chart
options are being investigated. Keep watching the AAVSO website and the
AAVSO Discussion Group for chart information.
Report Object to the AAVSO as: 0914-29 N PYX 05
Observations Reported to the AAVSO: March 5.259 UT, (14.0 V, ASAS; 14.260,
12.4 V, ASAS; 15.00, 12.6 V, ASAS; 16.00, 12.8 V, ASAS; 16.451, 12.8 CR
(unfiltered CCD, red magnitude).
Notes (from IAU Circular 8495):
a. H. Yamaoka provides the following position end figures by K. Itagaki,
Teppo-cho, Yamagata, Japan, using a 0.60-m reflector, from his own
unfiltered CCD image taken on March 16.451 UT: 58.50s, 37.0".
b. H. Yamaoka adds that Itagaki's position is close to the northern star
(blue mag about 18.0) of a close double on the Digitized Sky Survey.
Congratulations to ASAS and H. Haseda on their independent discoveries!
2. NEW PROBABLE CATACLYSMIC VARIABLE: 0523+62 RXSJ053234 (BERNHARD01)
Full name: 1RXSJ053234.9+624755 (= BERNHARD01)
Description: This new CV in Camelopardalis was discovered some time ago by
Klaus Bernhard, Linz, Austria. It is reported to be in outburst by Patrick
Schmeer, Bischmisheim, Germany, and confirmed in outburst by Wolfgang
Renz, Karlsruhe, Germany, according to the following observations:
March 15.82 UT, <13.1, Schmeer
16.819, 11.9, Schmeer
16.823 UT, 12.0, Renz
Position: R.A. (2000): 05h 32m 33.87s Decl. (2000): +62o 47' 52.1", by
P. Schmeer
Chart(s): A chart prepared by M. Simonsen is available to
[cvnet-discussion] group members at the url below:
http://groups.yahoo.com/group/cvnet-discussion/files/
Watch the AAVSO website and discussion group for further information on
availability of this chart.
Report Object to the AAVSO as: 0523+62 RXSJ053234
Note: Time-series CCD photometry is particularly requested to help
determine the CV sub-type of this new CV. Visual observations are also
strongly encouraged!
3. FOLLOW-UP ON REQUEST TO MONITOR U GEMINORUM
Over the past several months, on behalf of our colleague Dr. John
Cannizzo, NASA Goddard Space Flight Center, we had asked you to monitor
the cataclysmic variable U Gem closely and report its going into outburst.
He had planned to observe U Gem on its next outburst with RXTE on a Target
Of Opportunity (TOO) observing campaign.
When U Gem went into outburst on February 20, 2005, you notified us
promptly and we notified Dr. Cannizzo at once (fortunately he was home on
a Sunday afternoon!). He contacted the RXTE scheduling team immediately,
but, most unfortunately, they were not able to divert from the target they
were observing in time for the satellite observations to be at the phase
Dr. Cannizzo wanted to study, so the request was cancelled. Please don't
be discouraged that the TOO observations did not happen this time. It is
disappointing, but sometimes TOO observations simply are not feasible when
the target presents itself.
It is hoped Dr. Cannizzo will be able to obtain satellite observations of
U Gem when it next goes into outburst, please continue to monitor U Gem
closely, and inform us immediately when it brightens to magnitude 13.5 or
brighter. Both visual and CCD observations are encouraged. NEW CHARTS FOR
U GEM WERE ISSUED IN FEBRUARY 2004, and are available on the AAVSO
website. Please make sure you are using these latest charts. If you do not
have access to the website, please contact Headquarters and ask for the
new charts to be sent to you.
The tremendous coverage - both visual and CCD - of U Gem during these past
months, and particularly during the last outburst, is a real testimony to
your dedication, enthusiasm, and patience. On behalf of Dr. Cannizzo, and
personally, thank you very, very much.
SUBMIT OBSERVATIONS TO THE AAVSO
We encourage observers to submit observations via our web site (online
data submission tool WebObs), or by email in AAVSO format to
observations@aavso.org. If you do not have AAVSO Observer Initials, please
contact Headquarters so we may assign them to you. The answering machine
at AAVSO Headquarters is on nights and weekends; use our charge-free
number (888-802-STAR = 888-802-7827) to report your observations, or
report them via fax (617-354-0665).
Many thanks for your valuable astronomical contributions and your efforts.
Good observing!
Elizabeth O. Waagen
Senior Technical Assistant