We explore a scenario in which metal-poor globular clusters (GCs) are enriched by the first supernovae in the universe. If the first stars in a 107 Msolar dark...
-
PublicationThe Metallicity of Pregalactic Globular Clusters: The Observational Consequences of the First Stars
-
PublicationThe metallicity-period-mass diagram of low-mass exoplanets
The number of exoplanet detections continues to grow following the development of better instruments and missions. Key steps for the understanding of these...
-
PublicationThe methane ice rich surface of large TNO 2005 FY_9: a Pluto-twin in the trans-neptunian belt?
Context: .The population of known large trans-neptunian objects (TNOs) is growing very fast and the knowledge of their physical properties is a key issue to...
-
PublicationThe Mice at play in the CALIFA survey. A case study of a gas-rich major merger between first passage and coalescence
We present optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (≳1011 M⊙) gas-rich spirals NGC 4676A and B...
-
PublicationThe microvariability characteristics of OJ 287.
We present the results of the study of visible (UBVRIZ) intra-night microvariability in the blazar OJ 287. Useful observations (at least four integrations in a...
-
PublicationThe Mid- and Far-Infrared Spectral Energy Distribution of Seyfert Galaxies
Not Available
-
PublicationThe Mid-Infrared Emission of Seyfert Galaxies: A New Analysis of ISOCAM Data
We present mid-infrared data of a sample of 57 AGNs obtained with the instrument ISOCAM on board the Infrared Space Observatory (ISO) satellite. The images were...
-
PublicationThe Milky Way bar and bulge revealed by APOGEE and Gaia EDR3
We investigate the inner regions of the Milky Way using data from APOGEE and Gaia EDR3. Our inner Galactic sample has more than 26 500 stars within |X Gal|< 5...
-
PublicationThe Milky Way bar pattern speed using Hercules and Gaia DR3
The distribution of moving groups in the solar neighbourhood has been used to constrain dynamical properties of the Milky Way for decades. The kinematic...