A high-mass X-ray binary descended from an ultra-stripped supernova

Author:

Richardson Noel D.ORCID,Pavao Clarissa M.,Eldridge Jan J.ORCID,Pablo Herbert,Chené André-Nicolas,Wysocki PeterORCID,Gies Douglas R.,Younes GeorgeORCID,Hare Jeremy

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference39 articles.

1. De, K. et al. A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary. Science 362, 201 (2018).

2. Tauris, T. M., Langer, N. & Podsiadlowski, P. Ultra-stripped supernovae: progenitors and fate. Mon. Not. R. Astron. Soc. 451, 2123 (2015).

3. Barthelmy, S. D. et al. Swift detection of a likely new SGR: SGR 0755-2933. The Astronomer’s Telegram 8831, 1 (2016).

4. Archibald, R. F. et al. Swift XRT observations of SGR J0755-2933. The Astronomer’s Telegram 8868, 1 (2016).

5. Surnis, M. P. et al. Upper limits on the pulsed radio emission from SGR candidate SGR 0755-2933. The Astronomer’s Telegram 8943, 1 (2016).

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