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[vsnet-chat 2477] Re: [AAVSO-DIS] GRB notification process
- Date: Thu, 23 Dec 1999 00:37:56 +0900 (JST)
- To: aavso-discussion@informer2.cis.McMaster.CA
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 2477] Re: [AAVSO-DIS] GRB notification process
- Cc: vsnet-chat
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: [AAVSO-DIS] GRB notification process
> Berto drew our attention to this possible GRB/SNe association.
> There has been much discussion on this case in the literature
> and at meetings. The background was that when the GRB went off,
> SAX found two X-ray sources in the error box. One was centered
> on SN 1998bw; the other was a fading X-ray source (classical
> counterpart to other GRBs). This second source was ignored,
> and the SNe was speculated to be the counterpart, especially
> since the SNe occurred within a day or so of the GRB. Many
> models were produced, showing how a hypernovae (a more massive
> star than a supernovae progenitor) could produce beamed gamma
> rays, and spectra also showed 1998bw to be unusual. Still,
> the classical source was ignored.
I don't know what is the current consensus of this event (probably none
yet reached), but I have heard the existtence of the second "fading X-ray
source" was not so significant as was prevously claimed to be, by later
examination of the discovery data.
Regards,
Taichi Kato
Return to Daisaku Nogami
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