Zobrazeno 1 - 10
of 70
pro vyhledávání: '"Kapoor, R. C."'
Autor:
Kapoor, R. C.1 rck@iiap.res.in
Publikováno v:
Journal of Astronomical History & Heritage. Jun2024, Vol. 27 Issue 2, p273-289. 17p.
Autor:
Orchiston, Wayne1,2 wayne.orchiston@gmail.com, Kapoor, R. C.3 rck@iiap.res.in
Publikováno v:
Journal of Astronomical History & Heritage. Jun2024, Vol. 27 Issue 2, p363-386. 24p.
Autor:
Orchiston, Wayne1,2 wayne.orchiston@gmail.com, Kapoor, R. C.3 rckapoor@outlook.com
Publikováno v:
Journal of Astronomical History & Heritage. Dec2023, Vol. 26 Issue 4, p923-952. 30p.
Autor:
Kapoor, R. C.1 rckapoor@outlook.com;rck@iiap.res.in
Publikováno v:
Journal of Astronomical History & Heritage. Sep2023, Vol. 26 Issue 3, p599-620. 22p.
Autor:
Kapoor, R. C.1 rckapoor@outlook.com;rck@iiap.res.in
Publikováno v:
Journal of Astronomical History & Heritage. Sep2023, Vol. 26 Issue 3, p683-700. 18p.
Autor:
Kapoor, R. C.1 rckapoor@outlook.com
Publikováno v:
Journal of Astronomical History & Heritage. Sep2024, Vol. 27 Issue 3, p693-694. 2p.
Autor:
Kapoor, R. C., Shukre, C. S.
We present a new method for investigating emission altitudes of radio pulsar core and conal components by attributing them different altitudes and by providing a framework to understand the resulting longitude offsets between them which are frequentl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205429
Autor:
Kapoor, R. C., Shukre, C. S.
Publikováno v:
Astronomy and Astrophysics, 375, 405-410 (2001)
A remarkably precise observational relation for pulse core component widths of radio pulsars is used to derive stringent limits on pulsar radii, strongly indicating that pulsars are strange stars rather than neutron stars. This is achieved by inclusi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0011386
Autor:
Kapoor, R. C.
Publikováno v:
Current Science, 2017 Jul 01. 113(1), 173-179.
Externí odkaz:
http://www.jstor.org/stable/26163925
Autor:
Kapoor, R. C.
Publikováno v:
Current Science, 2016 Jun . 110(12), 2309-2314.
Externí odkaz:
http://www.jstor.org/stable/24908481