Santander, Miguel, 1979-
Miguel Santander astrophysicien ou astrophysicienne, écrivain ou écrivaine de science-fiction, vulgarisateur ou vulgarisatrice scientifique, chercheur ou chercheuse et astronome
VIAF ID: 260850144 (Personal)
Permalink: http://viaf.org/viaf/260850144
Preferred Forms
- 100 0 _ ‡a Miguel Santander ‡c astrophysicien ou astrophysicienne, écrivain ou écrivaine de science-fiction, vulgarisateur ou vulgarisatrice scientifique, chercheur ou chercheuse et astronome
- 100 1 _ ‡a Santander, Miguel ‡d 1979-
- 100 1 _ ‡a Santander, Miguel ‡d 1979-
-
4xx's: Alternate Name Forms (10)
Works
Title | Sources |
---|---|
36 | |
[Concentration of trace elements in children from northern Chile] | |
[Deficit of essential elements in children of Antofagasta. Analysis by neutron activation] | |
Direct measurement of stellar angular diameters by the VERITAS Cherenkov telescopes | |
Discovery of methyl silane and confirmation of silyl cyanide in IRC +10216. | |
The double-degenerate, super-Chandrasekhar nucleus of the planetary nebula Henize 2-428. | |
La Epopeya de los amantes | |
Estudio de la evolución dinámica, mecanismos de colimación y estrellas centrales de nebulosas bipolares | |
Exilium : primer impacto | |
Gas infall and possible circumstellar rotation in R Leo | |
High-resolution observations of IRAS 08544–4431: Detection of a disk orbiting a post-AGB star and of a slow disk wind. | |
IceCube-190504A: Swift-XRT Follow-up Observations | |
INTEGRAL pointed follow-up of IceCube-171106A | |
Joint Swift XRT and NuSTAR Observations of TXS 0506+056 | |
El legado de Prometeo | |
The maser-emitting structure and time variability of the SiS lines J = 14-13 and 15-14 in IRC+10216 | |
Optical photometry of TX0506+056 | |
Premio UPC 2012 novela corta de ciencia ficción | |
Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1 | |
Swift observation of a new gamma-ray source associated with 1WHSP J104516.2+275133 | |
Through the magnifying glass: ALMA acute viewing of the intricate nebular architecture of OH231.8+4.2. |