Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Lucas M. Valenzuela"'
Autor:
Caro Derkenne, Richard M McDermid, Adriano Poci, J Trevor Mendel, Francesco D’Eugenio, Seyoung Jeon, Rhea-Silvia Remus, Sabine Bellstedt, Andrew J Battisti, Joss Bland-Hawthorn, Anna Ferré-Mateu, Caroline Foster, K E Harborne, Claudia D P Lagos, Yingjie Peng, Piyush Sharda, Gauri Sharma, Sarah Sweet, Kim-Vy H Tran, Lucas M Valenzuela, Sam Vaughan, Emily Wisnioski, Sukyoung K Yi
We investigate the impact of environment on the internal mass distribution of galaxies using the Middle Ages Galaxy Properties with Integral field spectroscopy (MAGPI) survey. We use 2D resolved stellar kinematics to construct Jeans dynamical models
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9fcc36de10c9165e122f07cfc811688f
http://arxiv.org/abs/2306.09630
http://arxiv.org/abs/2306.09630
Autor:
Lucas M. Valenzuela, Benjamin P. Moster, Rhea-Silvia Remus, Joseph A. O'Leary, Andreas Burkert
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 505:5815-5832
We present an empirical model for the number of globular clusters (GCs) in galaxies based on recent data showing a tight relationship between dark matter halo virial masses and GC numbers. While a simple base model forming GCs in low-mass haloes repr
Autor:
Stefano de Nicola, Roberto P. Saglia, Jens Thomas, Claudia Pulsoni, Matthias Kluge, Ralf Bender, Lucas M. Valenzuela, Rhea-Silvia Remus
We discuss the statistical distribution of galaxy shapes and viewing angles under the assumption of triaxiality by deprojecting observed Surface Brightness (SB) profiles of 56 Brightest Cluster Galaxies coming from a recently published large deep-pho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::54c11d2a7460f5f1331bb116a62180e6
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We describe a revised procedure for the numerical simulation of planetary nebulae luminosity functions (PNLF), improving on previous work (M\'endez & Soffner 1997). The procedure now is based on new H-burning post-AGB evolutionary tracks (Miller Bert
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::213392b91aaa9fba4b6a8c637ec908fc
Publikováno v:
Astrophysical Journal; 12/10/2019, Vol. 887 Issue 1, p1-1, 1p