A multiwavelength study of the remnant of nova GK Persei

Author:

Anupama G. C.,Kantharia N. G.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. Relativistic electron populations in Cassiopeia A

2. The nebular remnant and quiescent spectrum of Nova GK Persei

3. Balman, S. 2002, in Classical Nova Explosions, ed. M. Hernanz, & J. Jose, AIP Conf. Ser., 637, 365

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1. Unveiling the 3D structure of nova shells with MUSE: The case of RR Pic;Astronomy & Astrophysics;2024-01

2. The intermediate polar cataclysmic variable GK Persei 120 years after the nova explosion: a first dynamical mass study;Monthly Notices of the Royal Astronomical Society;2021-09-10

3. Distance mapping applied to four well-known planetary nebulae and a nova shell;Monthly Notices of the Royal Astronomical Society;2020-01-13

4. Measuring the Expansion and Age of the Nova Shell IPHASX J210204.7+471015;Monthly Notices of the Royal Astronomical Society;2018-12-18

5. Multimission observations of the old nova GK Per during the 2015 outburst;Monthly Notices of the Royal Astronomical Society;2017-04-06

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