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[vsnet-obs 6042] Southern observations of 13/14/15 June 97
- Date: Sun, 15 Jun 1997 11:27:14 +0200
- To: observations@aavso.org, vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-obs 6042] Southern observations of 13/14/15 June 97
- Disclaimer: The CSIR exercises no editorial control over E-mail messages originating in the organisation and the views in this message are therefore not necessarily those of the CSIR and/or its employees.
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- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Visual observations for Southern variables with the apogee 40x
120 from Pretoria:
good seeing with 55% moon on the early night observations.
Star UT Magn
cvs
VZ Tuc 14.1 <12.3
HD5980 14.1 10.9
WX Cet 14.1 <11.9
WX Hyi 14.1 <12.5
VW Hyi 14.102 10.5
IX Vel 13.7 9.5
CU Vel 13.713 11.7
CU Vel 14.710 11.7 eleventh night of outburst
T Pyx 13.7 <12.5
V436 Cen 13.7 <12.2
V442 cen 13.7 <12.4
RX Cru 13.7 10.8
BV Cen 13.7 <12.4
Z Aps 13.7 11.7
GW Lib 13.8 <12.5
U Sco 13.8 <12.8
V4334 Sgr 13.9 11.2
V745 Sco 13.9 <12.2
V4338 Sgr 13.9 <12.5
V394 CrA 13.9 <12.1
V725 Sgr 13.9 12.3
V2905 Sgr 13.9 11.6
V4074 Sgr 13.9 12.1
V3804 Sgr 13.9 12.4
V3941 Sgr 13.9 <12.4
FN Sgr 14.0 11.3
V4368 Sgr 14.0 10.1
RZ Gru 14.1 12.2
RXJ2353 14.1 <12.0
N Sco 97 13.955 11.5
N Sco 97 14.075 11.6
N Sco 97 15.013 11.6
rcbs
SY Hyi 14.1 12.1
Z Cir 13.7 12.1
V618 Sgr 13.9 <12.6
WX CrA 13.9 11.7
V1860 Sgr 13.9 12.4
U Aqr 14.1 11.5
Some comments:
on the CU Vel observations:
having adequate and visually 'correct' sequences on the chart,
estimates on CU Vel feel rather 'satisfying'. They are felt to be
precise, meaning they would repeat by the same observer on
different occasions. With CU Vel fading, the consecutive 11.7
estimates (24 hours separated) must indicate effects of superhump
activity.
on N Sco observations:
quite the opposite is felt... I am looking forward to the HIC system
for magnitudes.
Regards,
Berto Monard / MLF