Feedback-driven winds from star formation or active galactic nuclei might be a relevant channel for the abrupt quenching of star formation in massive galaxies...
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NewsA titanic interstellar medium ejection from a massive starburst galaxy
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NewsAbout metallicity variations in the local Galactic interstellar medium
In this work we discuss and confront recent results on metallicity variations in the local interstellar medium, obtained from observations of H II regions by...
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EventActividades por el Día Internacional de la Mujer y la Niña en la Ciencia
Desde el año 2015, a iniciativa de la Asamblea General de las Naciones Unidas, el 11 de febrero conmemora el Día Internacional de la Mujer y la Niña en la...
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NewsAn ionised bubble powered by a proto-cluster at z = 6.5
We show herein that a proto-cluster of Lyα emitting galaxies, spectroscopically confirmed at redshift 6.5, produces a remarkable number of ionising continuum...
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NewsAn ultraviolet wind in a neutron star X-ray binary transient
All disc-accreting astrophysical objects produce powerful disc winds. In compact binaries containing neutron stars or black holes, accretion often takes place...
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DocumentAnexo IV-BV21
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NewsAre ultra-diffuse galaxies Milky Way-sized?
Now almost 70 years since its introduction, the effective or half-light radius has become a very popular choice for characterising galaxy size. However, the...
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NewsAre ultra-diffuse galaxies structurally similar to low-surface-brightness galaxies?
A central question regarding ultra-diffuse galaxies (UDGs) is whether they are in a separate category from low-surface-brightness (LSB) galaxies, or just their...
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NewsBlack holes modulate star formation in neighboring galaxies
Every massive galaxy hosts a black hole in its center. Both the size and the mass of these black holes is negligible compared to the host galaxy, millions of...