HIP 13962 – THE POSSIBLE FORMER MEMBER OF BINARY SYSTEM WITH SUPERNOVA

HIP 13962 – THE POSSIBLE FORMER MEMBER OF BINARY SYSTEM WITH SUPERNOVA

The run away supergiant star HIP13962 (spectral type G0Ia) was recently pointed as a possible former binary companion of young pulsar PSRJ0826+2637. The spectraof HIP13962 wereo btained in Haute-Provence observatory (France), in Bohuynsan observatory (Korea), and also in NARIT (Thailand) with1.9, 1....

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Bibliographic Details
Main Authors:	V. Yushchenko, A. Yushchenko, V. Gopka, A. Shavrina, V. Kovtyukh, K. S. Hong, D. Mkrtichian, N. A-Thano
Format:	Article
Language:	English
Published:	Odessa I. I. Mechnykov National University 2016-12-01
Series:	Odessa Astronomical Publications
Online Access:	http://oap.onu.edu.ua/article/view/85238

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