Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Bryan A. Terrazas"'
Autor:
Minjung Park, Sirio Belli, Charlie Conroy, Benjamin D. Johnson, Rebecca L. Davies, Joel Leja, Sandro Tacchella, J. Trevor Mendel, Chloë Benton, Letizia Bugiani, Razieh Emami, Amir H. Khoram, Yijia Li, Gabriel Maheson, Elijah P. Mathews, Rohan P. Naidu, Erica J. Nelson, Bryan A. Terrazas, Rainer Weinberger
Publikováno v:
The Astrophysical Journal, Vol 976, Iss 1, p 72 (2024)
Massive quiescent galaxies in the young Universe are expected to be quenched rapidly, but it is unclear whether they all experience starbursts before quenching and what physical mechanism drives rapid quenching. We study 14 massive quiescent galaxies
Externí odkaz:
https://doaj.org/article/06f816bf67e44287b03adb8f56dc4572
Autor:
Osase Omoruyi, Grant R. Tremblay, Francoise Combes, Timothy A. Davis, Michael D. Gladders, Alexey Vikhlinin, Paul Nulsen, Preeti Kharb, Stefi A. Baum, Christopher P. O’Dea, Keren Sharon, Bryan A. Terrazas, Rebecca Nevin, Aimee L. Schechter, John A. Zuhone, Michael McDonald, Hakon Dahle, Matthew B. Bayliss, Thomas Connor, Michael Florian, Jane R. Rigby, Sravani Vaddi
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 1, p 1 (2024)
With two central galaxies engaged in a major merger and a remarkable chain of 19 young stellar superclusters wound around them in projection, the galaxy cluster SDSS J1531+3414 ( z = 0.335) offers an excellent laboratory to study the interplay betwee
Externí odkaz:
https://doaj.org/article/d8ba79c486a8475ab675a6f5d477b184
Autor:
Abigail I Hartley, Erica J Nelson, Katherine A Suess, Alex M Garcia, Minjung Park, Lars Hernquist, Rachel Bezanson, Rebecca Nevin, Annalisa Pillepich, Aimee L Schechter, Bryan A Terrazas, Paul Torrey, Sarah Wellons, Katherine E Whitaker, Christina C Williams
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:3138-3144
We identify the first quiescent galaxies in TNG300, the largest volume of the IllustrisTNG cosmological simulation suite, and explore their quenching processes and time evolution to z=0. We find that the first quiescent galaxies with stellar masses M
Autor:
Rosalind E. Skelton, Paul Torrey, Bryan A. Terrazas, Sandro Tacchella, Katherine E. Whitaker, Lamiya Mowla, Benedikt Diemer, Federico Marinacci, Rüdiger Pakmor, Dylan Nelson, Joel Leja, Rebecca Nevin, Mark Vogelsberger, Lars Hernquist, Rainer Weinberger, Joshua S. Speagle, Benjamin D. Johnson, Erica J. Nelson, Volker Springel, Stijn Wuyts, Gabriel B. Brammer, Annalisa Pillepich, Rachel Cochrane, Blakesley Burkhart, Pieter van Dokkum
Publikováno v:
Nelson, E J, Tacchella, S, Diemer, B, Leja, J, Hernquist, L, Whitaker, K E, Weinberger, R, Pillepich, A, Nelson, D, Terrazas, B A, Nevin, R, Brammer, G B, Burkhart, B, Cochrane, R K, van Dokkum, P, Johnson, B D, Marinacci, F, Mowla, L, Pakmor, R, Skelton, R E, Speagle, J, Springel, V, Torrey, P, Vogelsberger, M & Wuyts, S 2021, ' Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 1, pp. 219-235 . https://doi.org/10.1093/mnras/stab2131
Nelson, E J, Tacchella, S, Diemer, B, Leja, J, Hernquist, L, Whitaker, K E, Weinberger, R, Pillepich, A, Nelson, D, Terrazas, B A, Nevin, R, Brammer, G B, Burkhart, B, Cochrane, R K, Van Dokkum, P, Johnson, B D, Marinacci, F, Mowla, L, Pakmor, R, Skelton, R E, Speagle, J, Springel, V, Torrey, P, Vogelsberger, M & Wuyts, S 2021, ' Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 1, stab2131, pp. 219-235 . https://doi.org/10.1093/mnras/stab2131
Nelson, E J, Tacchella, S, Diemer, B, Leja, J, Hernquist, L, Whitaker, K E, Weinberger, R, Pillepich, A, Nelson, D, Terrazas, B A, Nevin, R, Brammer, G B, Burkhart, B, Cochrane, R K, Van Dokkum, P, Johnson, B D, Marinacci, F, Mowla, L, Pakmor, R, Skelton, R E, Speagle, J, Springel, V, Torrey, P, Vogelsberger, M & Wuyts, S 2021, ' Spatially resolved star formation and inside-out quenching in the TNG50 simulation and 3D-HST observations ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 1, stab2131, pp. 219-235 . https://doi.org/10.1093/mnras/stab2131
We compare the star forming main sequence (SFMS) -- both integrated and resolved on 1kpc scales -- between the high-resolution TNG50 simulation of IllustrisTNG and observations from the 3D-HST slitless spectroscopic survey at z~1. Contrasting integra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e772c673fcfb9637c42138955ee00088
https://curis.ku.dk/portal/da/publications/spatially-resolved-star-formation-and-insideout-quenching-in-the-tng50-simulation-and-3dhst-observations(c36c0984-6d74-4cc4-9f7b-f6fb09154a5d).html
https://curis.ku.dk/portal/da/publications/spatially-resolved-star-formation-and-insideout-quenching-in-the-tng50-simulation-and-3dhst-observations(c36c0984-6d74-4cc4-9f7b-f6fb09154a5d).html
Autor:
Robert Feldmann, Sarah Wellons, Claude André Faucher-Giguère, Philip F. Hopkins, Bryan A. Terrazas, Daniel Anglés-Alcázar, Matthew E. Orr, T. K. Chan, Rachel S. Somerville, Greg L. Bryan, Cameron Hummels, Kung-Yi Su, Dušan Kereš, Christopher C. Hayward, Jonathan Stern
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2021, Vol.507(1), pp.175-204 [Peer Reviewed Journal]
Without additional heating, radiative cooling of gas in the halos of massive galaxies (Milky Way and above) produces cold gas or stars in excess of that observed. Previous work suggested that AGN jets are likely required, but the form of jet energy r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::065eecd3d2d3469963e10e83bb7dbe8e
https://doi.org/10.1093/mnras/stab2021
https://doi.org/10.1093/mnras/stab2021
Autor:
Mélanie Habouzit, Yuan Li, Annalisa Pillepich, Rainer Weinberger, Rachel S. Somerville, Eric F. Bell, Lars Hernquist, Bryan A. Terrazas, Mark Vogelsberger, Dylan Nelson, Shy Genel
Publikováno v:
arXiv
Supermassive black hole feedback is thought to be responsible for the lack of star formation, or quiescence, in a significant fraction of galaxies. We explore how observable correlations between the specific star formation rate (sSFR), stellar mass (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4d76ac2b05584d874de9a2ef7c988d28
https://hdl.handle.net/1721.1/132566
https://hdl.handle.net/1721.1/132566
Autor:
Sandro Tacchella, Fengshan Liu, Dale D. Kocevski, Fangzhou Jiang, Bryan A. Terrazas, Mauro Giavalisco, Jerome J. Fang, Viraj Pandya, S. M. Faber, Zhijian Luo, Guillermo Barro, A. van der Wel, Samir Salim, Chenggang Shu, Marc Huertas-Company, Aldo Rodríguez-Puebla, David C. Koo, Lin Lin, Henry C. Ferguson, Joel R. Primack, Rachel S. Somerville, Joanna Woo, Camilla Pacifici, Avishai Dekel, Zhu Chen, Eric F. Bell, Susan A. Kassin, Hassen M. Yesuf, Yicheng Guo, Yifei Luo
Existing models of galaxy formation have not yet explained striking correlations between structure and star-formation activity in galaxies, notably the sloped and moving boundaries that divide star-forming from quenched galaxies in key structural dia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38d8e768cd00de6a46f53f6460d1849a
http://arxiv.org/abs/1909.10817
http://arxiv.org/abs/1909.10817
Autor:
Melanie Habouzit, Lars Hernquist, Dylan Nelson, Mark Vogelsberger, Shy Genel, Rachel S. Somerville, Chung-Pei Ma, Yuan Li, Annalisa Pillepich, Eric F. Bell, Bryan A. Terrazas, Vicente Rodriguez-Gomez, Ruediger Pakmor, Rainer Weinberger
Publikováno v:
The Astrophysical Journal. 895:102
We study black hole - host galaxy correlations, and the relation between the over-massiveness (the distance from the average $M_{BH}-\sigma$ relation) of super-massive black holes (SMBHs) and star formation histories of their host galaxies in the Ill
Autor:
Bruno M. B. Henriques, Bryan A. Terrazas, Simon J. Lilly, Simon D. M. White, Asa F. L. Bluck, Eric F. Bell
We use the Henriques et al. (2015) version of the Munich galaxy formation model (L-GALAXIES) to investigate why the halo and stellar mass scales above which galaxies are quenched are constant with redshift and coincide with the scale where baryons ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e171fa4361a675da5632b4fcd0781377
http://arxiv.org/abs/1809.01154
http://arxiv.org/abs/1809.01154
We present a relationship between the black hole mass, stellar mass, and star formation rate of a diverse group of 91 galaxies with dynamically-measured black hole masses. For our sample of galaxies with a variety of morphologies and other galactic p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da629b58868a156ec4f058a9f215f357
http://arxiv.org/abs/1707.01097
http://arxiv.org/abs/1707.01097