Chapuzón cósmico: astronomical workshops for children
We present a set of six Astronomy outreach workshops for children called ''Chapuzón cósmico''. These workshops took place at the Museo de la Ciencia y el Cosmos...
Characterising Planetary Nebulae in the Large Magellanic Clouds
Planetary nebulae (PNe) represent the final link in the chain of the gas and dust enrichment of low- and intermediate-mass stars. We present a comprehensive...
Characterising six solar analogues observed by Kepler, K2, and Hermes
The Sun is a cornerstone of stellar astrophysics, offering a uniquely detailed benchmark due to its proximity. However, our ability to observe it spans only a...
Characterising the atmosphere of ultra hot Jupiters: MASCARA-2b
Ultra hot Jupiters orbit very close to their host star and consequently receive strong irradiation that makes their atmospheric chemistry different from the...
Characterising the colour and vertical structure of Saturn's haze using observations from the VLT/MUSE instrument
Saturn's atmosphere is characterised by a thick yellow haze that envelopes its entire surface. What causes this haze to be yellow, however, remains unknown. We...