The Pinwheel Galaxy, M101 // Wolfgang Reissenberger
In this image is the supernova SN 2023ixf. Can you spot it?
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The Pinwheel Galaxy, M101 // Wolfgang Reissenberger
In this image is the supernova SN 2023ixf. Can you spot it?
The Pinwheel Galaxy (M101) and NGC 5474 (right) // Sabine Leidinger
Included is the recent supernova SN 2023ixf! Can you find it?
The newly discovered supernova SN 2023ixf in the nearby Pinwheel Galaxy (M101) // Michael Bauer
This is the nearest supernova to Earth in a decade at just about 22.5 million lightyears away!
The Pinwheel Galaxy, M101 // Tony Jerig
Included is the bright supernova SN 2023ixf!
Descubierta una misteriosa supernova que desafía todas las teorías
Mientras se examinaba una supernova cercana con el telescopio espacial de rayos gamma Fermi de la NASA, los científicos han descubierto algo muy misterioso… Se descubrió que la supernova, denominada SN 2023ixf, carece por completo de las emisiones de rayos gamma que deberían estar presentes cuando las partículas de rayos cósmicos se aceleran a velocidades cercanas a la de la luz. Este es un…
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Two articles published in 'The Astrophysical Journal Letters' report as many studies on the supernova cataloged as SN 2023ixf. Two teams of
Two articles published in "The Astrophysical Journal Letters" report as many studies on the supernova cataloged as SN 2023ixf. Two teams of researchers with members in common examined the evolution of this supernova discovered in the so-called Pinwheel Galaxy. To do this, they used various instruments including some from the Center for Astrophysics (CFA) Harvard & Smithsonian which allowed observations in different electromagnetic bands. The results were different from what was expected from the explosion of a massive star with a delay in the time of the peak of the light pulse just before the explosion. The conclusion is that this was due to the presence of dense materials ejected from the star in the year preceding the supernova.
Due articoli pubblicati sulla rivista 'The Astrophysical Journal Letters' riportano altrettanti studi sulla supernova catalogata come SN 202
Due articoli pubblicati sulla rivista "The Astrophysical Journal Letters" riportano altrettanti studi sulla supernova catalogata come SN 2023ixf. Due team di ricercatori con vari membri in comune hanno esaminato l'evoluzione di questa supernova scoperta nella cosiddetta Galassia Girandola. Per farlo, hanno usato diversi strumenti tra i quali alcuni del Center for Astrophysics (Cfa) Harvard & Smithsonian che hanno permesso osservazioni in diverse bande elettromagnetiche. I risultati sono stati diversi rispetto a quanto ci si aspettava dall'esplosione di una stella massiccia con un ritardo nel momento del picco dell'impulso luminoso appena prima dell'esplosione. La conclusione è che ciò è stato dovuto alla presenza di materiali densi espulsi dalla stella nell'anno precedente alla supernova.
some girls maybe party on solstice. others spend the shortest night of the year photographing distant supernovae