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[vsnet-obs 2602] CL Scorpii e.o.
- Date: Tue, 16 Apr 1996 10:21:37 +0200
- To: observations@aavso.org, vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Berto Monard <LagMonar@csir.co.za>
- Subject: [vsnet-obs 2602] CL Scorpii e.o.
- Disclaimer: The views expressed in this message are those of the author, and not necessarily those of the CSIR and/or it's employees.
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Hi,
due to malfunctioning of my e-mail system I have been unable to report
earlier.
The following observations were done on CL SCO using the sequences
of RR SCO (RASNZ 1973):
UT Magn
13.1 11.7
16.1 11.7
Comparing those values to other observers's I wonder if the sequences
of the above starchart are still OK?
Other 'interesting' observations:
AR Pavonis (this Z And system is more than 1 magnitude brighter than
normal)
13.1 10.1
16.1 10.2
RS Telescopii (this RCB type is nearly 1 magnitude fainter than normal)
13.1 10.6
16.1 10.6
V854 Cen (an RCB type that is brightening again)
16.1 8.5
Best regards from Pretoria,
Berto Monard (MLF)
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