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[vsnet-obs 5873] Southern observations for 27 May 97
- Date: Wed, 28 May 1997 10:11:20 +0200
- To: observations@aavso.org, vsnet-obs@kusastro.kyoto-u.ac.jp, Guy@tahq.demon.co.uk, dave@telf-ast.demon.co.uk
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-obs 5873] Southern observations for 27 May 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
Results of visual observations performed with the apogee 40x120
from Pretoria on 27 May 1997:
semi-cloudy with clear patches at first, open and hazy later. Cold
that it was!
Star UT Magn
cvs
HS Pup 27.7 <12.2
DY Pup 27.7 <12.3
RX Pup 27.7 10.8
IX Vel 27.7 9.6
VZ Pyx 27.7 <12.4
CU Vel 27.7 <12.4
CQ Vel 27.7 <12.1
T Pyx 27.7 <12.5
WY Vel 27.7 8.6
V436 Cen 27.8 <12.2
V442 Cen 27.8 <12.2
SY Mus 27.7 10.7
CP Cru 27.7 <12.1
TV Crv 27.8 <12.5
BI Cru 27.7 10.8
BP Cru 27.7 11.1
AP Cru 27.7 <12.0
RX Cru 27.7 10.3
EX Hya 27.8 <12.2
BV Cen 27.8 <12.4
EK TrA 27.8 <12.2
GW Lib 27.8 <12.8
V341 Nor 27.8 <12.2
U Sco 27.8 <12.3
V4334 Sgr 27.8 <12.2 was N Sgr 90
V745 Sco 27.8 <12.2
V394 CrA 27.8 <12.2
V1830 Sgr 27.8 <12.2
V4074 Sgr 27.8 12.0
AR Pav 27.8 11.3 back to its 'old' form?!
V2905 Sgr 27.8 11.5 still bright
V441 Sgr 27.8 <12.1
V3804 Sgr 27.8 12.4
V3941 Sgr 27.8 <12.2
V3890 Sgr 27.8 <12.2
FN Sgr 27.8 11.4
V4368 Sgr 27.8 10.3 was Wakuda's object
V3885 Sgr 27.8 10.3
RR Tel 27.8 10.9
rcbs
UW Cen 27.8 <12.2
Y Mus 27.8 10.4
V854 Cen 27.8 7.5
S Aps 27.8 10.4
RT Nor 27.8 10.5
RZ Nor 27.8 11.5
WX CrA 27.8 11.5
V3795 Sgr 27.8 11.0
RS Tel 27.8 10.2
V1860 Sgr 27.8 12.2
GU Sgr 27.8 10.4
RY Sgr 27.8 6.5
Remarks:
according to the new listing of variables some of my 'old' rcb:'s
were uncovered as belonging to other classes. They have been
taken off this reporting list. It concerns NSV 7344 (now V1026 Sco
and of type IA) and HDE 320156 (also known as LSS 4300 and
now V1037 Sco of type PV Tel).
AR Pav's present brightness at magnitude 11.3 is similar to before
its excursion through a maximum around 10.1 (as a result of high
activity (presumably) in '96) and a minimum near 13 (as a result of
an eclipse during early '97).
Will it again stay at 11.3 for the next couple of years???
Best regards,
Berto Monard / MLF