Showing 1 to 7 of 7 results
First Photographic Evidence of Type Ia Supernova's Double Detonation
Astronomers using the European Southern Observatory's Very Large Telescope have obtained the first photographic evidence of a Type Ia supernova, a double-detonation event 160,000 light-years away in the Large Magellanic Cloud, revealing two concentric calcium shells expanding outwards, confirming th...
First Photographic Evidence of Type Ia Supernova's Double Detonation
Astronomers using the European Southern Observatory's Very Large Telescope have obtained the first photographic evidence of a Type Ia supernova, a double-detonation event 160,000 light-years away in the Large Magellanic Cloud, revealing two concentric calcium shells expanding outwards, confirming th...
Progress
32% Bias Score
Discovery of X-ray-Emitting Long-Period Transient Challenges Stellar Evolution Theories
Astronomers detected ASKAP J1832-0911, a celestial object 15,000 light-years away, emitting bright flashes of radio waves and X-rays every 44 minutes; this is the first X-ray detection associated with a long-period transient (LPT), challenging existing theories on stellar evolution and suggesting a ...
Discovery of X-ray-Emitting Long-Period Transient Challenges Stellar Evolution Theories
Astronomers detected ASKAP J1832-0911, a celestial object 15,000 light-years away, emitting bright flashes of radio waves and X-rays every 44 minutes; this is the first X-ray detection associated with a long-period transient (LPT), challenging existing theories on stellar evolution and suggesting a ...
Progress
20% Bias Score
Binary Star System Unveiled as Source of Milky Way's Cosmic Pulses
A binary star system, consisting of a white dwarf and a red dwarf orbiting each other every 125.5 minutes, located 1600 light-years from Earth in the constellation Ursa Major, has been identified as the source of previously mysterious two-hour radio pulses.
Binary Star System Unveiled as Source of Milky Way's Cosmic Pulses
A binary star system, consisting of a white dwarf and a red dwarf orbiting each other every 125.5 minutes, located 1600 light-years from Earth in the constellation Ursa Major, has been identified as the source of previously mysterious two-hour radio pulses.
Progress
20% Bias Score
Binary Star System Identified as Source of Milky Way's Mysterious Radio Pulses
Astronomers have identified a binary star system, ILTJ1101, comprising a white dwarf and a red dwarf star, as the source of mysterious, repeating radio pulses detected in the Ursa Major constellation; this discovery expands our understanding of radio pulse generation and challenges previous assumpti...
Binary Star System Identified as Source of Milky Way's Mysterious Radio Pulses
Astronomers have identified a binary star system, ILTJ1101, comprising a white dwarf and a red dwarf star, as the source of mysterious, repeating radio pulses detected in the Ursa Major constellation; this discovery expands our understanding of radio pulse generation and challenges previous assumpti...
Progress
12% Bias Score
Celestial Object's 44-Minute Radio and X-Ray Pulses Challenge Stellar Evolution Models
Astronomers detected ASKAP J1832-0911, a celestial object emitting two-minute-long radio waves and X-rays every 44 minutes, located 15,000 light-years from Earth; this challenges existing models of stellar evolution and opens new research avenues.
Celestial Object's 44-Minute Radio and X-Ray Pulses Challenge Stellar Evolution Models
Astronomers detected ASKAP J1832-0911, a celestial object emitting two-minute-long radio waves and X-rays every 44 minutes, located 15,000 light-years from Earth; this challenges existing models of stellar evolution and opens new research avenues.
Progress
24% Bias Score
Mysterious Celestial Object Emits Correlated X-rays and Radio Waves
An international team discovered a celestial object, ASKAP J1832−091, 15,000 light-years away in the Milky Way, emitting correlated X-rays and radio waves every 44 minutes during hyperactive phases lasting about a month, unlike any known Galactic object.
Mysterious Celestial Object Emits Correlated X-rays and Radio Waves
An international team discovered a celestial object, ASKAP J1832−091, 15,000 light-years away in the Milky Way, emitting correlated X-rays and radio waves every 44 minutes during hyperactive phases lasting about a month, unlike any known Galactic object.
Progress
32% Bias Score
Binary Star System Discovered as Source of Mysterious Radio Pulses
A binary star system, ILTJ1101, located 1600 light-years away in Ursa Major, emits repeating radio pulses every 125 minutes due to the interaction of a visible red dwarf and an unseen white dwarf star, marking the first such detection outside of magnetars.
Binary Star System Discovered as Source of Mysterious Radio Pulses
A binary star system, ILTJ1101, located 1600 light-years away in Ursa Major, emits repeating radio pulses every 125 minutes due to the interaction of a visible red dwarf and an unseen white dwarf star, marking the first such detection outside of magnetars.
Progress
20% Bias Score
Showing 1 to 7 of 7 results