 and CO(7-6) ALMA maps of the narrow (broad) emission HST imaging and narrow and broad components ALMA maps of ID2299. The top-left panel shows the HST-F814W imaging of the source, sampling the UV rest-frame emission from young stars. The top (bottom) rows show the CO(2-1), CO(5-4), [CI](2-1) and CO(7-6) ALMA maps of the narrow (broad) emission](/sites/default/files/styles/crop_cinemascope_32_13_to_1920px/public/images/news/nature_210111.png?h=843cd5de&itok=xJbqcCUA)
An international study published in Nature Astronomy, in which the Instituto de Astrofísica de Canarias (IAC) is a participant, suggests that the feedback winds do not have a direct impact on braking
An international study published in Nature Astronomy, in which the Instituto de Astrofísica de Canarias (IAC) is a participant, suggests that the feedback winds do not have a direct impact on braking
Studying the universe needs a major effort of scientific research and in the development of astronomical instruments.
Astrophysical research is the main objective of the IAC and corresponds to the Research Area the elaboration and development of Research Projects in the field of Astrophysics and related areas.We aim to strengthen and consolidate the position of the IAC as an international reference centre for research in Astrophysics. On regard of the research activity, it results in an effective increase in scientific production and international impact in recent years.
In order to advance observational astrophysics needs new instruments at the forefront of technology, which offers a constant challenge to produce new development in technology which can often be applied to many other fields of general utility.