https://jhare.net/about/https://jhare.net/wp-content/uploads/2017/01/943718_2239900088146_2076328677_n.jpg943718_2239900088146_2076328677_n2025-06-25T20:14:20+00:00weekly0.6https://jhare.net/blog-2/2024-11-19T16:18:58+00:00weekly0.6https://jhare.net/contact/2024-05-08T01:02:33+00:00weekly0.6https://jhare.net/ads-refereed-publications/https://jhare.net/wp-content/uploads/2019/09/b1259_both.pngb1259_bothhttps://jhare.net/wp-content/uploads/2019/09/b1259_2014_2017.pngb1259_2014_2017Image showing the motion of the blob over 3 observations(colored in red, green, and blue) spanning ~3 years during the 2014-2017 binary cycle.https://jhare.net/wp-content/uploads/2018/09/gc01_nasaapod.jpegGC01_NasaAPODhttps://jhare.net/wp-content/uploads/2017/01/high-res_glimpse.jpeghigh-res_Glimpsehttps://jhare.net/wp-content/uploads/2017/01/noname.pngnonameImage showing the motion of the blob over 3 observations(colored in red, green, and blue) spanning ~3 years during the 2010-2014 binary cycle.https://jhare.net/wp-content/uploads/2017/01/psrb1259.jpgThe double star system PSR B1259-63/LS 2883 - or B1259 for short - contains a star about 30 times as massive as the Sun and a pulsar, an ultra-dense neutron star left behind when an even more massive star underwent a supernova explosion2024-04-28T14:30:21+00:00weekly0.6https://jhare.net/sgr0755/2020-10-12T20:01:40+00:00weekly0.6https://jhare.net/3fgl-j1016/2019-03-13T17:13:53+00:00weekly0.6https://jhare.net/2018/11/08/installing-heasoft-6-25-from-source-on-mac-os-high-sierra-v-10-13-6/2018-11-08T20:13:02+00:00monthlyhttps://jhare.net/2017/01/24/first-blog-post/2017-10-28T17:49:06+00:00monthlyhttps://jhare.net/research/2017-02-03T07:10:32+00:00weekly0.6https://jhare.netdaily1.02025-06-25T20:14:20+00:00