Tag Archive for 'CK Vulpeculae'

CK Vulpeculae resides in the constellation Vulpecula. It is just below the star Albireo, the head of Cygnus, the swan. That location is inside the Summer Triangle of bright stars, which is now high in the south after nightfall. The star is approximately 2,200 light-years from Earth. Image credit: ALMA / ESO / NAOJ / NRAO / Eyres et al.

ALMA Discovers New Type of Stellar Collision

Oct 10, 2018 by News Staff

Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers found evidence that a white dwarf and a brown dwarf collided in a ‘blaze of...

An artist’s impression of the collision of two stars, like the ones that formed CK Vulpeculae. The inset illustrates the inner structure of one red giant before the merger. A thin layer of 26Al (brown) surrounds a helium core. An extended convective envelope (not to scale), which forms the outermost layer of the star, can mix material from inside the star to the surface, but it never reaches deep enough to dredge 26Al up to the surface. Only a collision with another star can disperse 26Al. Image credit: NRAO / AUI / NSF / S. Dagnello.

Radioactive Molecule Found in Stellar Merger Remnant

Aug 2, 2018 by News Staff

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) and the Northern Extended Millimeter Array (NOEMA) have made the first definitive...

This image shows the remnant of CK Vulpeculae; the image was created from a combination of visible-light images from the Gemini telescope, blue, a submillimeter map showing the dust from the SMA, green, and finally a map of the molecular emission from APEX and the SMA, red. Image credit: ESO / T. Kamiński.

Ground-Based Telescopes Reveal Secrets of Enigmatic Nova CK Vulpeculae

Mar 23, 2015 by News Staff

According to an international group of astronomers led by Dr Tomasz Kamiński of ESO and the Max Planck Institute for Radio Astronomy in Bonn, Germany,...