Observers find two stars so close together that they will end up by merging into 1 very massive star
A study of the binary system “MY Camelopardalis” published in the journalAstronomy & Astrophysics, shows that the most massive stars are formed by the merging of other smaller stars, as theoretical models predicted.
The second data release of the international project CALIFA - a survey of galaxies carried out at Calar Alto observatory – will take place today.
Performed at Calar Alto, CALIFA reaffirms to Calar Alto as a very competitive worldwide astronomical facility and highly productive.
Calar Alto Observatory took part on the European Night of the Researches with a roundtable and an exposition of anaglyph (3D images) showing the constellations, in collaboration with the Instituto Astrofísico de Andalucía (CSIC) and the Asociación de Amigos de Calar Alto.
Since July 2014, Calar Alto Observatory has a fireball detection station which is composed by five high sensitivity CCD cameras. These devices are monitoring the firmament during the whole night and allow automatic identification of meteoroids entering into our atmosphere. These meteoroids are falling material fragments from asteroids, comets or even other planets.
The systems installed at Calar Alto for the analysis of these interplanetary matter are part of the SMART project, developed under the scientific direction of Prof. José María Madiedo (Universidad de Huelva) in collaboration with the Instituto de Astrofísica de Andalucía (IAA-CSIC).
By clicking here you will go to the web page containing all the objects observed with this new system and with Calar Alto external surveillance webcams. That web page will be upgrade as soon as new fireballs are detected.
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