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- VSNET - An Intensive International Mailing List on Variable Stars
VSNET Collaboration news (posted to AstroAlert) VSNET 2001 VSNET 2000 If you are interested to join VSNET collaboration team, please send an e-mail to vsnet-adm@kusastro kyoto-u ac jp Welcome to the wild kingdom of e-mails! Owing to the server maintainance, on-line article archives and light curves will not be updated for a while
- VSNET Information - Kyoto U
Recently, many e-mails for subscription and unsubscription have been distributed via all three mailing lists of VSNET (vsnet, vsnet-alert, and vsnet-obs) However, such e-mails should be originally sent to VSNET administrators (vsnet-adm@kusastro kyoto-u ac jp)
- VSNET (国際変光星ネットワーク) 日本語ページ - Kyoto U
SOHO画像に姿を現したさそり座デルタ 日本語MLを開始しました 参加受付中! 日本語ML (vsnet-j)投稿一覧! CCD vs 眼視観測!? (Message Nextをクリックすると続きが読めます) 個々の変光星データ (変光星図ほか)をお探しの方はこちらへ VSNET 2001 VSNET 2000
- VSNET - An Intensive International Mailing List on Variable Stars
vsnet-recent-nova vsnet-recent-pec vsnet-recent-polar vsnet-recent-qso vsnet-recent-rcb vsnet-recent-rr vsnet-recent-rscvn vsnet-recent-sdor vsnet-recent-sn vsnet-recent-sss vsnet-recent-swsex vsnet-recent-symbio vsnet-recent-ug vsnet-recent-ugss vsnet-recent-ugsu vsnet-recent-ugz vsnet-recent-unknown vsnet-recent-vyscl vsnet-recent-xn vsnet
- VSNET: World-Leading Network on Variable Stars
[Announcement on VSNET] Scientific Activities of VSNET [2001] [2002] [2003] You can see all activities of the VSNET champions by sending an e-mail "SUBSCRIBE vsnet champion everything" to vsnet-adm@kusastro kyoto-u ac jp [Mail Archive] [Data Search] [Individual Objects] Latest vsnet-alert (archived) message!
- CI Aql = Recurrent Nova Aql 1917,2000 - Kyoto U
Now the identity of the nova by Takamizawa and Yamamoto (issued as IAUC 7409) with CI Aql (nova 1917) is firmly established, please use the designation AQLCI (in the VSNET format) in reporting to vsnet-obs (use CI Aql in other situations)
- The 2001 Superoutburst of WZ Sge: The King of Dwarf Novae! - Kyoto U
We have put on the VSNET WZ Sge page the figures representing the recent variations of the hump and eclipse profiles Please note the dramatic change of (super?)humps (phase and amplitude) and eclipses (phase and profile) across the rebrightening
- SN 2002ap in M74
The preliminary analysis of the spectrum (See vsnet-alert 7120) reveals very unusual feature, which resembles to that of "hypernova"! The follow-up observation in all wavelength is surely, strongly, highly recommended for this unique and very interesting exploding object!
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