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[vsnet-chat 1576] Re: NL: stars in Name List 74
- Date: Mon, 25 Jan 1999 08:44:40 +0200
- To: tkato@kusastro.kyoto-u.ac.jp, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Berto Monard <lagmonar@csir.co.za>
- Subject: [vsnet-chat 1576] Re: NL: stars in Name List 74
- 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-chat@kusastro.kyoto-u.ac.jp
Dear Kato-san,
I remember a previous GCVS list with NL(:)s where a number of what I
thought to be confirmed Z And systems were tabled.
Of special personal interest was Hen 3-916 which I have been
monitoring some time ago.
I looked up its 'colours' in USNO_A2.0 and found it to be a reddish
star (as was measured by U Munari earlier) while other neighbouring
stars were definitely more 'white' proving it was not from a reddening
effect.
I just wonder why they are now considered NL(:)
Regards,
Berto
Pretoria
>>> Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> 01/25 4:55 AM >>>
NL: stars in Name List 74
One of our colleagues have noticed there are several Hipparcos
variables
newly classified as NL: in the 74-th special name list.
The list of NL: stars
FH Leo 8.33-8.62 Hp, spec. F8
PQ Ser 8.12-8.22 Hp, spec. F0
V1440 Aql 8.55-8.67 Hp, spec. B8, eclipsong binary with a period
of 1.84d
V2151 Cyg 12.08-12.89 Hp, spec. DA
I wonder why these stars have been classified as NL: (NL stars are
usually
considered as a subclass of cataclysmic variables). I presume at
least
the F-type spectrum (without emission lines) is incompatible with this
variability type.
Regards,
Taichi Kato
Return to Daisaku Nogami
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