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The most complete portrait of a supernova ever

The most complete portrait of a supernova ever
phys.org - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from phys.org Daily Mail and Mail on Sunday newspapers.

Israel
Erez-zimmerman
Ido-irani
Avishay-gal
Weizmann-institute-of-science-liverpool-telescope
Weizmann-institute-of-science
Baltimore-space-telescope-science-institute
Liverpool-telescope
Weizmann-institute
Keck-observatory
Milky-way
Avishay-gal-yam

Minutes-duration optical flares with supernova luminosities

In recent years, certain luminous extragalactic optical transients have been observed to last only a few days1. Their short observed duration implies a different powering mechanism from the most common luminous extragalactic transients (supernovae), whose timescale is weeks2. Some short-duration transients, most notably AT2018cow (ref. 3), show blue optical colours and bright radio and X-ray emission4. Several AT2018cow-like transients have shown hints of a long-lived embedded energy source5, such as X-ray variability6,7, prolonged ultraviolet emission8, a tentative X-ray quasiperiodic oscillation9,10 and large energies coupled to fast (but subrelativistic) radio-emitting ejecta11,12. Here we report observations of minutes-duration optical flares in the aftermath of an AT2018cow-like transient, AT2022tsd (the ‘Tasmanian Devil’). The flares occur over a period of months, are highly energetic and are probably nonthermal, implying that they arise from a near-relativistic

South-korea
Compton
Illinois
United-states
Willingale
Essex
United-kingdom
Chicago
Cambridge
Cambridgeshire
Kuin
Ch-ungch-ong-bukto

A rotating white dwarf shows different compositions on its opposite faces

White dwarfs, the extremely dense remnants left behind by most stars after their death, are characterized by a mass comparable to that of the Sun compressed into the size of an Earth-like planet. In the resulting strong gravity, heavy elements sink towards the centre and the upper layer of the atmosphere contains only the lightest element present, usually hydrogen or helium1,2. Several mechanisms compete with gravitational settling to change a white dwarf’s surface composition as it cools3, and the fraction of white dwarfs with helium atmospheres is known to increase by a factor of about 2.5 below a temperature of about 30,000 kelvin4–8; therefore, some white dwarfs that appear to have hydrogen-dominated atmospheres above 30,000 kelvin are bound to transition to be helium-dominated as they cool below it. Here we report observations of ZTF J203349.8+322901.1, a transitioning white dwarf with two faces: one side of its atmosphere is dominated by hydrogen and

Cambridge
Cambridgeshire
United-kingdom
Montreal
Quebec
Canada
Netherlands
Douglas-gough
Gran-telescopio-canarias
Gentile-fusillo
Holland-publishing-co
Astronomical-society-of-the-pacific-conference-series

Hawaii astronomers say this burned-out star is 'two-faced.' (It's not an insult)

Hawaii astronomers say this burned-out star is 'two-faced.' (It's not an insult)
hawaiinewsnow.com - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from hawaiinewsnow.com Daily Mail and Mail on Sunday newspapers.

San-diego
California
United-states
Ilaria-caiazzo
Keck-observatory
Mauna-kea
Low-resolution-imaging-spectrometer
Kecki-telescope
Near-infared-echelletee-spectrograph

Two-Faced Star Exposed: Unusual White Dwarf Star Is Made Of Hydrogen On One Side And Helium On The Other

Two-Faced Star Exposed: Unusual White Dwarf Star Is Made Of Hydrogen On One Side And Helium On The Other
spaceref.com - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from spaceref.com Daily Mail and Mail on Sunday newspapers.

California
United-states
Spain
Hawaii
California-institute-of-technology
Maunakea
Chile
San-diego
Cuba
Hawaiian
Caltech-palomar
Gran-telescopio-canarias

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