It may interest you
-
A team of scientists led by the Observatory of Munich University and the Instituto de Astrofísica de Canarias have obtained direct visualization of the process of feeding the supermassive black hole at the centre of the Andromeda galaxy. The study reveals the existence of long filamentary structures of gas and dust which move in a spiral starting at a distance from the black hole and ending up at the black hole itself. The results, which have been published in the Astrophysical Journal, were obtained using images from the Hubble and Spitzer space telescopes. The Andromeda Galaxy, which isAdvertised on
-
From 14 to 16 February, the second scientific meeting of the Laboratory for Innovation in Opto-Mechanics (LIOM) will be held at the IACTEC building managed by the Instituto de Astrofísica de Canarias (IAC) in the Science and Technology Park of La Laguna (Tenerife). This project is dedicated to the development of new optical and mechanical technologies that will form part of the next generation of telescopes capable of detecting biomarkers on exoplanets. One year after its creation, the IAC's Laboratory for Innovation in Opto-Mechanics (LIOM), is holding its second international meetingAdvertised on
-
An international collaboration, with the participation of the Instituto de Astrofísica de Canarias (IAC), determines with an unprecedented level of precision the mass, age and rotation profile of the core of a massive pulsating star. Known as HD 192575, it has been observed by the NASA space telescope TESS continuously for more than a year. The results shed new light on how such stars are internally structured and how they evolve until their death, when they explode as supernovae and form neutron stars and black holes. The scientific team has also used observations made with the MercatorAdvertised on