En esta tesis se explora el estrecho límite que separa las estrellas más masivas que acaban su vida explotando como una supernova y aquellas menos masivas que dan lugar a una nebulosa planetaria. Para ello se ha estudiado, mediante espectroscopía de alta resolución, una muestra de estrellas evolucionadas presentes en cúmulos abiertos jóvenes.
openaire +1 more source
The chemistry in circumstellar envelopes of evolved stars: following the origin of the elements to the origin of life. [PDF]
Ziurys LM.
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The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment. [PDF]
Cox NLJ +29 more
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A new species of supergiant <i>Bathynomus</i> A. Milne-Edwards, 1879 (Isopoda: Cirolanidae) from the Paracel Islands, South China Sea. [PDF]
Huang MC, Kawai T.
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Hints of the existence of C-rich massive evolved stars. [PDF]
Quintana-Lacaci G +8 more
europepmc +1 more source
Herschel/HIFI observations of the circumstellar ammonia lines in IRC+10216. [PDF]
Schmidt MR +16 more
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Electronic structure of metal oxide dications with ammonia ligands and their reactivity towards the selective conversion of methane to methanol. [PDF]
Claveau EE, Miliordos E.
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High-energy Gamma Rays from the Milky Way: Three-dimensional Spatial Models for the Cosmic-Ray and Radiation Field Densities in the Interstellar Medium. [PDF]
Porter TA +2 more
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Achieving high-density states through shock-wave loading of precompressed samples. [PDF]
Jeanloz R +7 more
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