DQ Herculis, or Nova Herculis 1934, was a slow, bright nova occurring in the northern constellation of Hercules in December 1934. This cataclysmic variable...

In astronomy, an intermediate polar (also called a DQ Herculis Star) is a type of cataclysmic variable, binary star system with a white dwarf and a cool...

These binary systems usually have orbital periods of under 2.5 hours. DQ Herculis systems are interacting binaries in which a low-mass star transfers mass...

in 1943. T Aurigae is classified as a slow nova, similar to DQ Herculis. Like DQ Herculis, WZ Sagittae, Nova Persei 1901 and Nova Aquilae 1918, it is...

13 December 1934 when amateur astronomer J. P. M. Prentice discovered DQ Herculis from the town. Just before midday on Friday 31 January 1941, a solitary...

Martell, P. (2010-05-07). "Spectral Mapping of the Intermediate Polar Dq Herculis". The Astronomical Journal. 139 (6): 2542–2556. arXiv:1005.1612. Bibcode:2010AJ...

Spin-down and Ultrafast Outflows of the Highly Pulsed Supersoft Source of Nova Herculis 2021". The Astrophysical Journal Letters. 922 (2): L42. arXiv:2110.14058...

rather than forming a disc. DQ Herculis, also called 'intermediate polars', have a slightly weaker magnetic field than AM Herculis stars; there is an accretion...

AE Aquarii is a cataclysmic variable binary star of the DQ Herculis type. Based upon parallax measurements, the system is located at a distance of about...

soft X-rays coming from the primary. This system was identified as a DQ Herculis variable by J. Patterson and associates in 1994 – also known as an intermediate...