[vsnet-chat 600] WX CrA sequence (Monard)

[Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>]

From owner-vsnet@kusastro.kyoto-u.ac.jp Tue Sep  9 16:25 JST 1997
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Date: Tue, 09 Sep 1997 09:57:35 +0300
From: Berto Monard <lagmonar@csir.co.za>
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Subject: [vsnet 1105] WX CrA / sequences
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Hi Southern observers,

I want to return to some unfinished business: ie sequences for the
RCB variable WX CrA. 

Applying the Tycho measures to the WX CrA field, most of the
brighter RASNZ chart letter sequences can be quantified. With an
estimated magnitude of 11.3 for star l and VSNET measures for the
fainter stars we have a suitable comparison set for WX CrA. 
It looks as follows:

letter    V mag
d      10.8  
f      107
h     110
l      113
m    121
n     125
p     126
q     130
r      133
s      139

I can precisely trace my old WX CrA estimates to the new standard
by subtracting 0,3. 
Surely if we were to accept the new set, we could all convert our
WX CrA estimates ?
What do you think? Please comment whatever way...
I also hope to sollicit some reactions from the VSS of RASNZ!

Regards,

Berto Monard / MLF
Pretoria

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