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A Shortcut to Calculate SPAM Limb-darkening CoefficientsWe release a new grid of stellar limb-darkening coefficients (LDCs, using the quadratic, power-2 and claret-4 laws) and intensity profiles for the Kepler, U, B, V and R passbands, based on STAGGER model atmospheres. The data can be downloaded from Zenodo: https://doi.org/10.5281/zenodo.5593162. We compare the newly released LDCs, computed byMorello, Giuseppe et al.
Fecha de publicación:
102021 -
A young spectroscopic binary in a quintuple system part of the Local AssociationContext. Double-lined spectroscopic (SB2) binaries allow us to obtain a direct determination of the masses of their components, which is essential to test stellar models. Although these objects only provide a lower limit for the mass, they are more abundant than their eclipsing counterparts as they are not as strongly limited by the inclination ofCardona Guillén, Carlos et al.
Fecha de publicación:
102021 -
Capturing dual AGN activity and kiloparsec-scale outflows in IRAS 20210+1121The most standard scenario for the evolution of massive galaxies across cosmic time assumes a correspondence based on the interplay between active galactic nuclei (AGN) feedback, which injects large amounts of energy into the host environment, and galaxy mergers, with their ability to trigger massive star formation events and accretion ontoSaturni, F. G. et al.
Fecha de publicación:
102021 -
CARMENES detection of the Ca II infrared triplet and possible evidence of He I in the atmosphere of WASP-76bUltra-hot Jupiters are highly irradiated gas giants with equilibrium temperatures typically higher than 2000 K. Atmospheric studies of these planets have shown that their transmission spectra are rich in metal lines, with some of these metals being ionised due to the extreme temperatures. Here, we use two transit observations of WASP-76b obtainedCasasayas-Barris, N. et al.
Fecha de publicación:
102021 -
Euclid: Constraining dark energy coupled to electromagnetism using astrophysical and laboratory dataIn physically realistic, scalar-field-based dynamical dark energy models (including, e.g., quintessence), one naturally expects the scalar field to couple to the rest of the model's degrees of freedom. In particular, a coupling to the electromagnetic sector leads to a time (redshift) dependence in the fine-structure constant and a violation of theMartinelli, M. et al.
Fecha de publicación:
102021