Intermediate Polars is a subclass of cataclysmic variable stars characterized by a magnetic white dwarf primary that accretes material from a companion star via an accretion disk, with the distinguishing feature that the white dwarf’s rotational period is intermediate between synchronous rotation and very rapid, non-synchronous spin, leading to observable quasi-periodic oscillations in its electromagnetic emission.
230
Publications
7.5K
Citations
412
Authors
247
Institutions
Publications per year
2017–2026
30
Variants
Dq Herculis Stars
Publications
230
1–5 of 230
Authors
412
- CH
17
h-index
- AJ
16
h-index
- KM
15
h-index
- DAD. A. H. Buckley
South African Radio Astronomy Observatory, South Africa
16 publications · 412 citations
14
h-index
- BT
11
h-index
1–5 of 412
Institutions
247
University of Leicester
Leicester, United Kingdom
20 h-index
37 publications
1.5K citations
South African Radio Astronomy Observatory
Cape Town, South Africa
16 h-index
41 publications
1.1K citations
Keele University
Newcastle-under-Lyme, United Kingdom
16 h-index
30 publications
946 citations
Goddard Space Flight Center
Greenbelt, United States
16 h-index
22 publications
664 citations
The Open University
Milton Keynes, United Kingdom
15 h-index
26 publications
1K citations
University of Warwick
Coventry, United Kingdom
15 h-index
44 publications
1.2K citations
University of Maryland, Baltimore County
Baltimore, United States
14 h-index
18 publications
444 citations
University of Cape Town
Rondebosch, South Africa
14 h-index
35 publications
932 citations
1–8 of 247
Venues
- Monthly Notices of the Royal Astronomical Society
110 publications · 3.6K citations
35
h-index
- Astronomy and Astrophysics
34 publications · 1.2K citations
21
h-index
- The Astrophysical Journal
ApJ · 29 publications · 1K citations
19
h-index
- The Astronomical Journal
AJ · 12 publications · 477 citations
12
h-index
- Publications of the Astronomical Society of the Pacific
PASP · 7 publications · 163 citations
7
h-index
1–5