
In February 2016 the dwarf nova SS Cyg anomalous outburst lasted for more than 3 weeks.
Dwarf novae (SS Cyg-like objects, which contain a Sun-like star orbiting a white dwarf star) are well known for their repeated, low-level, bursting behaviour (called "outbursts") but they have never been observed exhibiting behaviour on anything like the scale of rapid flares before.
Outbursts have previously been seen in white dwarfs, neutron stars and even enormous black holes residing in different galaxies. Such stars mainly feed on gas from their companion stars via accretion (where a large amount of gas is accumulated and builds up through gravitational force). Occasionally, these stars "throw up" some of the gas in the form of jets, which are powerful overflows of gas restricted to a single, narrow, cone-like flow.
Initial observations of the SS Cyg activity in February 2016 were considered an atypical outburst, but later telescopic analysis uncovered the intriguing revelation of rapid flares. The most fascinating and unexpected behaviour was observed at radio wavelengths towards the end of the outburst, when a "giant" flare was observed. Lasting for less than 15 minutes, it had the energy of more than a million times the strongest solar flares. The level of radio data recorded from the flare is unprecedented in dwarf nova systems and consistent with that expected from a jet.















Comment: Test tube experimental habitation riding on waves of change.