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Radio Emission of Dwarf Novae

1989
With the recent detection of radio emission from dwarf novae a new channel of information on these semi-detached binaries has opened. The radiation is variable within days and highly polarized. Most likely it is emitted by some gyromagnetic process, which would allow to estimate the magnetic field.
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Southern Dwarf Novae

Vistas in Astronomy, 1988
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Automatic Classification of Dwarf Nova

2019
Dwarf nova is an abundant subtype of cataclysmic variable star with frequent eruptions. This binary star is a semi-close binary system consisting of a late dwarf secondary star with loch lobes and a White Dwarf host star. Finding more dwarf novae can help us to study the dynamic evolution of the system and many complex physical processes.
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A Jovian analogue orbiting a white dwarf star

Nature, 2021
J W Blackman   +2 more
exaly  

A giant planet candidate transiting a white dwarf

Nature, 2020
Andrew Vanderburg   +2 more
exaly  

A trail of dark-matter-free galaxies from a bullet-dwarf collision

Nature, 2022
Pieter van Dokkum   +2 more
exaly  

Dwarf Mongoose Optimization Algorithm

Computer Methods in Applied Mechanics and Engineering, 2022
Absalom E Ezugwu   +1 more
exaly  

DWARF 53 acts as a repressor of strigolactone signalling in rice

Nature, 2013
Xue Liu, Lei Wang, Xiangbing Meng
exaly  

GIBBERELLIN INSENSITIVE DWARF1 encodes a soluble receptor for gibberellin

Nature, 2005
Miyako Ueguchi-Tanaka   +2 more
exaly  

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