Zobrazeno 1 - 10
of 88
pro vyhledávání: '"Diaz, Jonathan"'
Autor:
Rivero-Yeverino, Daniela1 driveroy@hotmail.com, Higgins Payan-Diaz, Jonathan1, Inés López-García, Aída1, Sergio Papaqui-Tapia, José1, Gengyny Caballero-López, Chrystopherson1, Jesús Ríos-López, Juan1, David López-Romero, Carlos1, Yael Sánchez-Villalobos, Johav1, Ortega Jordá-Rodríguez, Elisa1, Álvarez-Rivera, Armando1, Villada-Villada, Erika1
Publikováno v:
Revista Alergia de Mexico. abr-jun2024, Vol. 71 Issue 2, p85-90. 6p.
Autor:
Omkumar, Abinaya O., Subramanian, Smitha, Niederhofer, Florian, Diaz, Jonathan, Cioni, Maria-Rosa L., Youssoufi, Dalal El, Bekki, Kenji, de Grijs, Richard, van Loon, Jacco Th.
Recent observational studies identified a foreground stellar sub-structure traced by red clump (RC) stars (~ 12 kpc in front of the main body) in the eastern regions of the Small Magellanic Cloud (SMC) and suggested that it formed during the formatio
Externí odkaz:
http://arxiv.org/abs/2010.02687
Autor:
Deeley, Simon, Drinkwater, Michael J., Sweet, Sarah M., Diaz, Jonathan, Bekki, Kenji, Couch, Warrick J., Forbes, Duncan A., Bland-Hawthorn, Joss, Bryant, Julia J., Croom, Scott, Cortese, Luca, Lawrence, Jon S., Lorente, Nuria, Medling, Anne M., Owers, Matt, Richards, Samuel N., van de Sande, Jesse
It has been proposed that S0 galaxies are either fading spirals or the result of galaxy mergers. The relative contribution of each pathway, and the environments in which they occur remains unknown. Here we investigate stellar and gas kinematics of 21
Externí odkaz:
http://arxiv.org/abs/2008.02426
Autor:
Schmidt, Thomas, Cioni, Maria-Rosa L., Niederhofer, Florian, Bekki, Kenji, Bell, Cameron P. M., de Grijs, Richard, Diaz, Jonathan, Youssoufi, Dalal El, Emerson, Jim, Groenewegen, Martin A. T., Ivanov, Valentin D., Matijevic, Gal, Oliveira, Joana M., Petr-Gotzens, Monika G., Queiroz, Anna B. A., Ripepi, Vincenzo, van Loon, Jacco Th.
Publikováno v:
A&A 641, A134 (2020)
The Magellanic Clouds are a nearby pair of interacting dwarf galaxies and satellites of the Milky Way. Studying their kinematic properties is essential to understanding their origin and dynamical evolution. They have prominent tidal features and the
Externí odkaz:
http://arxiv.org/abs/2006.03163
Autor:
Dolfi, Arianna, Forbes, Duncan A., Couch, Warrick J., Ferre-Mateu, Anna, Bellstedt, Sabine, Bekki, Kenji, Diaz, Jonathan, Romanowsky, Aaron J., Brodie, Jean P.
Publikováno v:
MNRAS 495, 1321-1339 (2020)
Using new and archival data, we study the kinematic properties of the nearest field S0 galaxy, NGC 3115, out to $\sim6.5$ half-light radii ($R_\mathrm{e}$) from its stars (integrated starlight), globular clusters (GCs) and planetary nebulae (PNe). We
Externí odkaz:
http://arxiv.org/abs/2004.09818
Akademický článek
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Publikováno v:
Proc. IAU 14 (2018) 130-133
Dwarf galaxies enable us to study the early phases of galaxy evolution and are key to many open questions about the hierarchical structure of the Universe. The Large and Small Magellanic Cloud (LMC and SMC) are the most luminous dwarf galaxy satellit
Externí odkaz:
http://arxiv.org/abs/1810.02701
Publikováno v:
OECD Education Working Papers / Documents de Travail de l'OCDE sur l'éducation; 5/16/2024, Issue 315, p1-95, 95p
Fluid mechanics provides the theoretical foundation for hydraulics, which focuses on the engineering uses of fluid properties. In fluid power, hydraulics is used for the generation, control, and transmission of power by the use of pressurized liquids
In the rest frame of the Local Group (LG), the total momentum of the Milky Way (MW) and Andromeda (M31) should balance to zero. We use this fact to constrain new solutions for the solar motion with respect to the LG centre-of-mass, the total mass of
Externí odkaz:
http://arxiv.org/abs/1405.3662