Publicación
Asphaltenes as model compounds of the UIBs/AIBs detected in various astrophysical objects. Part 2 – Natural bitumens asphaltenes carbonization
La Vía Láctea y el Grupo Local (MWLG)
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PublicaciónAsphaltenes as model compounds of the UIBs/AIBs detected in various astrophysical objects. Part 3: Petroleum asphaltenes high energy radiation processed
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PublicaciónAssessing spectra and thermal inversions due to TiO in hot Jupiter atmospheresRecent detections of thermal inversions in the dayside atmospheres of some hot Jupiters are motivating new avenues to understand the interplay between their...
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PublicaciónAssessing the Stellar Population and the Environment of an H II Region on the Far Side of the GalaxyWe have investigated the stellar and interstellar content of the distant star formation region IRAS 17591-2228 (WISE H II region GAL 007.47+0.06). It is...
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PublicaciónAsteroseismology of Massive Stars with the TESS Mission: The Runaway β Cep Pulsator PHL 346 = HN AqrWe report an analysis of the first known β Cep pulsator observed by the Transiting Exoplanet Survey Satellite (TESS) mission, the runaway star PHL 346 = HN Aqr...
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PublicaciónAstrometry with Carte du Ciel plates, San Fernando zone . II. CdC-SF: a precise proper motion catalogueContext. The historic plates of the Carte du Ciel, an international cooperative project launched in 1887, offer valuable first-epoch material for the...
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PublicaciónAstrophysical Parameters of LS 2883 and Implications for the PSR B1259-63 Gamma-ray BinaryOnly a few binary systems with compact objects display TeV emission. The physical properties of the companion stars represent basic input for understanding the...
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PublicaciónAsymmetrical tidal tails of open star clusters: stars crossing their cluster's práh<SUP>†</SUP> challenge Newtonian gravitationAfter their birth a significant fraction of all stars pass through the tidal threshold (práh) of their cluster of origin into the classical tidal tails. The...
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PublicaciónAsymptotic giant branch and super-asymptotic giant branch stars: modelling dust production at solar metallicityWe present dust yields for asymptotic giant branch (AGB) and super-asymptotic giant branch (SAGB) stars of solar metallicity. Stars with initial mass 1.5 M⊙ ≤...