
Prof of Astrophysics at @Usach, Oxford PhD. Leads @milenioyems, @astrociras, @astrodialogos, @conciertocielos, @BitacoraPlaneta
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ALT Representación artística de la vista a gran escala de FU Ori. En la imagen se aprecian los grandes chorros generados por la interacción entre los fuertes vientos estelares provenientes de la erupción y el envoltorio de gas y polvo remanente a partir del cual se formó la estrella. Al chocar con fuerza contra dicho envoltorio, el viento estelar arrastra el gas de CO detectado por ALMA. Créditos: NSF/NRAO/S. Dagnello

ALT This trio of images from NASA's Chandra X-Ray Observatory represents different aspects of black holes and black hole evolution. WR124 is an extremely bright, short-lived massive star known as a Wolf-Rayet that may collapse into a black hole in the future. SS 433 is a binary, or double system, containing a star like our Sun in orbit with either a neutron star or a black hole. The galaxy Centaurus A has an enormous black hole in its center that is sending a booming jet across the entire length of the galaxy.



















