The RCB star V854 Cen has just recovered from a deep decline that lasted
from January through July 2024. During September 2024 it gradually faded
again to visual magnitude 8.1, but it is not clear if this is the onset of
another deep decline. It has been cloudy for the past week here at
Heathcote NSW , so I have been unable to confirm the current state of V854
Cen. A check on this star would be appreciated - thanks.
Recent visual observations :
CENV854 20240923.381 …
[View More]81 WPX
CENV854 20240922.403 81 WPX
CENV854 20240921.398 80 WPX
CENV854 20240920.370 80 WPX
CENV854 20240919.397 80 WPX
CENV854 20240918.393 76 WPX
CENV854 20240915.398 76 WPX
CENV854 20240913.390 74 WPX
CENV854 20240909.440 74 WPX
CENV854 20240906.384 76 WPX
CENV854 20240905.383 74 WPX
CENV854 20240904.404 74 WPX
CENV854 20240902.401 74 WPX
CENV854 20240901.454 74 WPX
CENV854 20240831.374 75 WPX
Tks and regards
Peter Williams
Heathcote NSW
10x50mm binoculars
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TCP J17064645-3528079: new classical nova
TCP J17064645-3528079 was discovered by Koichi Itagaki on 2024-09-09.4363
UT at 11.4 mag.
I reported the optical spectrum of TCP J17064645-3528079 to ATel and
classified it as a new classical nova eruption.
https://www.astronomerstelegram.org/?read=16808
Further observations are encouraged.
Best regards,
Yusuke
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South African Astronomical Observatory, Postdoc fellow
Yusuke TAMPO
MAIL: tampo(a)…
[View More]kusastro.kyoto-u.ac.jp
MAIL: yusuke(a)saao.ac.za
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Dear colleagues,
I have just finished analysing my unfiltered CCD observations of
ASASSN-24fq, obtained on 2024, Aug 30/Sep 01 and Sep 01/02 at CBA
Extremadura Observatory using a 0.40-m f/5.1 telescope and SX-46 CCD camera
under clear skies.
The resulting light curve clearly shows the presence of regular superhumps
with an amplitude of 0.56 mag, establishing ASASSN-24fq as a new SU UMa-type
dwarf nova. A period analysis, using the ANOVA, Lomb-Scargle,
Generalized-Lomb-Scargle, PDM …
[View More]and Phase-binned AoV methods (Peranso 3.0)
yields a combined superhump period of 0.0590 +/- 0.0002d. The object was at
mag CV = 15.8 on Aug 13th.
Image calibration and photometry were done using my new photometry software
Phoranso 1.0.4.8, which allowed me to simultaenously measure several other
variables present in the FOV of this new SU UMa-type dwarf nova.
I will send my observations to AAVSO, CBA and VSNET for further analysis.
Best regards
Tonny
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Tonny Vanmunster
CBA Belgium Observatory
CBA Extremadura Observatory
http://www.cbabelgium.co <http://www.cbabelgium.com/> m
PERANSO : The Light Curve and Period Analysis Software
http://www.peranso.co <http://www.peranso.com/> m
PHORANSO: Photometric Reduction and Analysis Software *** NEW ***
http://www.phoranso.com <http://www.phoranso.com/>
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