Zobrazeno 1 - 10
of 390
pro vyhledávání: '"Campos, Marta"'
Autor:
Joschko, Philipp S., Kruijssen, J. M. Diederik, Trujillo-Gomez, Sebastian, Pfeffer, Joel L., Bastian, Nate, Crain, Robert A., Reina-Campos, Marta
We present a comprehensive analysis of globular cluster (GC) formation and evolution across the $34^3$ Mpc$^3$ volume of the E-MOSAICS galaxy formation simulations. Defining GCs as surviving, high-mass ($>10^5$ M$_\odot$) clusters, we analyse their f
Externí odkaz:
http://arxiv.org/abs/2412.04105
Most of the dynamical mass loss from star clusters is thought to be caused by the time-variability of the tidal field (``tidal shocks''). Systematic studies of tidal shocks have been hampered by the fact that each tidal history is unique, implying bo
Externí odkaz:
http://arxiv.org/abs/2410.16389
Stellar clusters are critical constituents within galaxies: they are the result of highest-density star formation, and through their spatially and temporally correlated feedback they regulate their host galaxy evolution. We present a novel numerical
Externí odkaz:
http://arxiv.org/abs/2408.04694
Deep JWST imaging of the giant galaxy cluster Abell 2744, at redshift $z=0.308$, is used to explore the features of its rich population of globular clusters (GCs), building on our initial survey of the system (Harris & Reina-Campos 2023). We use the
Externí odkaz:
http://arxiv.org/abs/2404.10813
Autor:
Diego, J. M., Li, Sung Kei, Amruth, Alfred, Meena, Ashish K., Broadhurst, Tom J., Kelly, Patrick L., Filippenko, Alexei V., Williams, Liliya L. R., Zitrin, Adi, Harris, William E., Reina-Campos, Marta, Giocoli, Carlo, Dai, Liang, Struble, Mitchell F., Treu, Tommaso, Fudamoto, Yoshinobu, Gilman, Daniel, Koekemoer, Anton M., Lim, Jeremy, Palencia, J. M., Sun, Fengwu, Windhorst, Rogier A.
Publikováno v:
A&A 689, A167 (2024)
Observations of caustic-crossing galaxies at redshift $0.7
Externí odkaz:
http://arxiv.org/abs/2404.08033
The advent of JWST (the James Webb Space Telescope) now allows entire star cluster populations to be imaged in galaxies at cosmologically significant redshifts, bringing with it the need to apply K-corrections to their magnitudes and colour indices.
Externí odkaz:
http://arxiv.org/abs/2310.02307
Autor:
Gensior, Jindra, Feldmann, Robert, Reina-Campos, Marta, Trujillo-Gomez, Sebastian, Mayer, Lucio, Keller, Benjamin W., Wetzel, Andrew, Kruijssen, J. M. Diederik, Hopkins, Philip F., Moreno, Jorge
Understanding what shapes the cold gas component of galaxies, which both provides the fuel for star formation and is strongly affected by the subsequent stellar feedback, is a crucial step towards a better understanding of galaxy evolution. Here, we
Externí odkaz:
http://arxiv.org/abs/2310.01482
The presence or absence of star clusters in galaxies, and the properties of star cluster populations compared to their host galaxy properties, are important observables for validating models of cluster formation, galaxy formation, and galaxy assembly
Externí odkaz:
http://arxiv.org/abs/2307.14423
JWST imaging of the rich galaxy cluster Abell 2744 at $z=0.308$ has been used by the UNCOVER team (Bezanson et al. 2022) to construct mosaic images in the NIRCAM filters. The exceptionally deep images in the ($F115W$, $F150W$, $F200W$) bands reveal a
Externí odkaz:
http://arxiv.org/abs/2307.14412
Massive star clusters are often used as tracers of galaxy formation and assembly. In order to do so, we must understand their properties at formation, and how those properties change with time, galactic environment, and galaxy assembly history. The t
Externí odkaz:
http://arxiv.org/abs/2306.17701