The characterization of stellar streams in the Milky Way halo can provide important observational constraints on the ΛCDM cosmological model, which posits that...
Characterizing the CARMENES input catalogue of M dwarfs with low-resolution spectroscopy: metallicity
In this contribution we summarise our science preparation activities to complete the CARMENES (http://carmenes.caha.es/) input catalogue of M dwarfs using low...
Characterizing the population of Asteroids in Cometary Orbits (ACOs)
The classification criterion between asteroids and comets has evolved in recent decades, but the main phenomenological distinction remains unchanged: comets are...
Chat with a Woman Astronomer. A pioneery activity organised by SEA's Comisi'on Mujer y Astronom'ia to commemorate 11F
Since 2015, February 11th commemorates the International Day of Women and Girls in Science, as set up by the United Nations. Such vindication is fully supported...
Chebbi region, Morocco: a testing site for future rover missions to Mars
In the future, new robotic missions will be launch toward Mars with the objective of studying this planet from its surface. Phoenix (2007), Mars Science...
Chemical Abundance Comparisons Between ASPCAP and Manual Analyses in Open Cluster Red Giants
The APOGEE Stellar Parameter and Chemical Abundance Pipeline (ASPCAP) has now produced individual chemical abundances for 15 different elements: C, N, O, Na, Mg...
Chemical abundance of 12 stars in open clusters (Carrera+, 2011)
Using high-resolution (R~30000), high-quality (S/N>=60 per pixel), we obtained spectra for twelve stars in four open clusters with the fibre spectrograph FOCES...