Modifying the Standard Disk Model for the Ultraviolet Spectral Analysis of Disk-dominated Cataclysmic Variables. I. The Novalikes MV Lyrae, BZ Camelopardalis, and V592 Cassiopeiae. [PDF]
Astrophys J, 2017 Godon P +4 more
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FUSE Spectroscopy of the Accreting Hot Components in Symbiotic Variables. [PDF]
Astron J, 2017 Sion EM +4 more
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Accretion in disks of dwarf novae
, 2019 Les novæ naines permettent, depuis presque 50 ans maintenant, de tester les modèles d’accrétion. Ces systèmes montrent des éruptions en optique d’une durée de l’ordre de la semaine avec des temps de récurrence de l’ordre du mois. Ces éruptions sont communément attribuées à une instabilité thermo-visqueuse au sein du disque d’accrétion entourant la ...
openaire +1 more source
The origin of ultra diffuse galaxies: stellar feedback and quenching. [PDF]
Mon Not R Astron Soc, 2018 Chan TK +7 more
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<i>HUBBLE SPACE TELESCOPE</i> FAR ULTRAVIOLET SPECTROSCOPY OF THE RECURRENT NOVA T PYXIDIS. [PDF]
Astrophys J Lett, 2014 Godon P +7 more
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The Evolution of Compact Binary Star Systems. [PDF]
Living Rev Relativ, 2014 Postnov KA, Yungelson LR.
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Characterization of the Priestia megaterium ZS-3 siderophore and studies on its growth-promoting effects. [PDF]
BMC MicrobiolZhu XX, Shi LN, Shi HM, Ye JR.
europepmc +1 more source
IRON: A KEY ELEMENT FOR UNDERSTANDING THE ORIGIN AND EVOLUTION OF INTERSTELLAR DUST. [PDF]
Astrophys J, 2016 Dwek E.
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The changing face of farmers' home gardens: a diachronic analysis from Sillian (Eastern Tyrol, Austria). [PDF]
J Ethnobiol Ethnomed, 2018 Vogl-Lukasser B, Vogl CR.
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