文件操作 - 1750921511.M232123P9359.mail.planetcloud-host.com,S=4711,W=4804:2,
返回文件管理
返回主菜单
删除本文件
文件: /var/vmail/bicar.it/stefano/cur/1750921511.M232123P9359.mail.planetcloud-host.com,S=4711,W=4804:2,
编辑文件内容
Return-Path: <atel@astronomerstelegram.org> Delivered-To: stefano@bicar.it Received: by mail.planetcloud-host.com (Postfix, from userid 1016) id 2AF1814CC1; Thu, 26 Jun 2025 09:05:11 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.4.0 (2014-02-07) on mail.planetcloud-host.com X-Spam-Level: X-Spam-Status: No, score=-0.0 required=7.0 tests=RCVD_IN_DNSWL_BLOCKED, RCVD_IN_VALIDITY_RPBL_BLOCKED,RCVD_IN_VALIDITY_SAFE_BLOCKED,SPF_HELO_NONE, SPF_PASS,URIBL_BLOCKED autolearn=disabled version=3.4.0 Received-SPF: Pass (sender SPF authorized) identity=mailfrom; client-ip=174.142.199.243; helo=server.astronomerstelegram.org; envelope-from=atel@astronomerstelegram.org; receiver=stefano@bicar.it Received: from server.astronomerstelegram.org (astronomerstelegram.org [174.142.199.243]) by mail.planetcloud-host.com (Postfix) with ESMTP id 4B5881452A for <stefano@bicar.it>; Thu, 26 Jun 2025 09:05:08 +0200 (CEST) Received: from server.astronomerstelegram.org (localhost [127.0.0.1]) by server.astronomerstelegram.org (Postfix) with ESMTP id AD36B28808CE for <stefano@bicar.it>; Thu, 26 Jun 2025 03:05:07 -0400 (EDT) To: stefano@bicar.it From: atel@astronomerstelegram.org Subject: ATel 17245 Message-Id: <20250626070507.AD36B28808CE@server.astronomerstelegram.org> Date: Thu, 26 Jun 2025 03:05:07 -0400 (EDT) ------------------------------------------------------------------------------ The Astronomer's Telegram is free to read, free to publish, free to use. Thanks to the support of our patrons, we can continue to keep it free. https://www.patreon.com/astronomerstel ------------------------------------------------------------------------------ The Astronomer's Telegram http://www.astronomerstelegram.org ------------------------------------------------------------------------------ Posted: Within the last 24 hours ============================================================================== ATEL #17245 ATEL #17245 Title: Return of the clocked burster GS 1826-238 Author: S. Iwata, N. Ota, T. Kita, K. Yamasaki, S. Tsuchiya, Y. Nakano, M. Ichibakase, T. Takeda, A. Aoyama, T. Takahashi (TUS/RIKEN), T. Tamagawa (RIKEN/TUS), T. Enoto (Kyoto U./RIKEN), W. Iwakiri (Chiba U.), T. Kitaguchi (RIKEN), C.-P. Hu (NCUE), T. Mihara (RIKEN), and the NinjaSat team Queries: tamagawa@riken.jp Posted: 25 Jun 2025; 10:32 UT Subjects:X-ray, Neutron Star, Transient NinjaSat observed the neutron star low-mass X-ray binary GS 1826-238 from 2025-06-23 13:05 UT to 2025-06-24 13:53 UT with a total exposure of 15.3 ks, and detected six Type-I X-ray bursts. The intervals between the first five bursts were nearly constant at approximately 1.6 hours, suggesting that GS 1826-238 may have entered a clocked burster state for the first time in 10 years. This is the shortest burst recurrence period ever measured for GS 1826-238 in its clocked burster state. GS 1826-238 remained in the hard state from 1996 until 2014. Between 1997 and 2007, it exhibited a clocked burster state with burst recurrence times of 3 to 6 hours, as reported by Thompson et al. (ApJ 681, 506, 2008), earning it the nickname "textbook burster". Around 2013, the source gradually brightened and transitioned to the soft state after 2014 (Fig. 12 in Asai et al., PASJ 74, 974, 2022). According to observations by Swift/BAT and MAXI, the intensity of GS 1826-238 gradually decreased since 2025-05-25, and transitioned back to the hard state on 2025-06-11. MAXI detected an X-ray burst from the source at 2025-06-20 14:37 UT. The burst onset times in MJD detected by NinjaSat are as follows: 60849.5464 60849.6135 60849.6805 60849.7474 60849.8125 60850.1932 Follow-up observations are encouraged, as GS 1826-238 is expected to remain in the hard state, with further clocked X-ray bursts. NinjaSat is a 6U-size X-ray CubeSat with Xe-filled proportional counters covering the energy range of 2-50 keV, focusing on agile observations of bright X-ray compact sources (Tamagawa et al., PASJ 77, 466, 2025). ------------------------------------------------------------------------------ Password Certification: Tatehiro Mihara (mihara@crab.riken.jp) https://www.astronomerstelegram.org/?read=17245 ============================================================================== ============================================================================== This is an automatically-generated notice. You can remove yourself permanently from receiving both the Daily Email Digest and Instant Email Notices from The Astronomer's Telegram by following this link: https://www.astronomerstelegram.org?unsubscribe&confirmation=a803d34e7ea924f9a4142bac00763549&address=stefano@bicar.it
修改文件时间
将文件时间修改为当前时间的前一年
删除文件