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[vsnet-alert 2727] NSV 08383 outburst / identification
- Date: Sun, 28 Feb 1999 15:53:35 +0200
- To: observations@aavso.org, vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-alert 2727] NSV 08383 outburst / identification
- 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.
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear VSNET readers,
I have identified NSV 08383 at its outburst position with star
USNO-A2.0 0225-27288943 at location 17 16 52.75 -65 32 47.1 This star
has a quiescent magnitude around 17.3 and B-R=0.7 which indicates the
blue colour of this object when compared to neighbouring stars of that
brightness level at quiescence.
I am confident that NSV08383 is a cv in outburst and not like V2323
Sgr and now recently V2038 Sgr which are non cvs and probable Mira
stars.
It would be very opportune to have this outburst confirmed and
specified by UBVRI (at least blue-red) measurements.
I propose the following comparison stars, calibrated vs a nearby GSPC
sequence, USNO-A2.0 refers:
0225-27292846 at 17 16 59.3 -65 32 17 , mag 143
0225-27286104 at 17 16 48.0 -65 31 36 , mag 139
0225-27277133 at 17 16 33.0 -65 31 42 , mag 147
These sequence stars are sufficiently 'white' to allow proper visual
comparison to bluish NSV 08383.
My recent observations using the above sequence
NSV08383 990223.99 <139 MLF
NSV08383 990227.11 142 MLF
NSV08383 990228.106 141 MLF
Best regards,
Berto Monard
Pretoria
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