Results 121 to 130 of about 262,815 (208)
The SAGA Survey. V. Modeling Satellite Systems around Milky Way–Mass Galaxies with Updated UniverseMachine
The Astrophysical JournalEnvironment plays a critical role in shaping the assembly of low-mass galaxies. Here, we use the U niverse M achine (UM) galaxy–halo connection framework and Data Release 3 of the Satellites Around Galactic Analogs (SAGA) Survey to place dwarf galaxy ...Yunchong Wang, Ethan O. Nadler, Yao-Yuan Mao, Risa H. Wechsler, Tom Abel, Peter Behroozi, Marla Geha, Yasmeen Asali, Mithi A. C. de los Reyes, Erin Kado-Fong, Nitya Kallivayalil, Erik J. Tollerud, Benjamin Weiner, John F. Wu +13 moredoaj +1 more sourceGLACE survey: OSIRIS/GTC multi-object spectroscopy of the rich galaxy cluster ZwCl 0024.0+1652 at
Context. Galaxy clusters are among the largest and densest structures in the Universe. Their high density generally increases the suppression of star formation, known as quenching, altering galaxy properties.
Aims. We study the quenching of emission-line Bernabé Cedrés, Mauro Gónzalez-Otero, Ángel Bongiovanni, Maritza A. Lara-López, Clara C. de la Casa, Jordi Cepa, Miguel Sánchez-Portal, Brisa Mancillas, Ricardo Pérez-Martínez, Daniel Espada, Ivan Valtchanov, Manuel Castillo-Fraile, Mónica I. Rodríguez, Carmen P. Padilla-Torres, Irene Cruz-González, Simon B. De Daniloff, Miguel Cerviño, José A. de Diego, Ana María Pérez-García, Zeleke Beyoro-Amado, Mirjana Pović, Gloria Torres-Ríos, J. Ignacio González-Serrano, Castalia Alenka Negrete, Perez-Garcia, A.M., Espada, D., Beyoro-Amado, Zeleke, De, Daniloff S.B., Lara-López, Maritza A., Sanchez-Portal, M., Torres-Ríos, Gloria, Perez-Martinez, R., Bongiovanni, A., de, la Casa C.C., Sánchez-Portal, Miguel, de Diego, José A., Castillo-Fraile, M., Cerviño, Miguel, Valtchanov, Ivan, Cruz-González, Irene, Espada, Daniel, De Daniloff, Simon B., Cepa, Jordi, Pérez-Martínez, Ricardo, Padilla-Torres, Carmen P., Rodríguez, Mónica I., Cedres, B., Pérez-García, Ana María, Valtchanov, I., de, Diego J.A., González-Otero, Mauro, de la Casa, Clara C., Cervino, M., Padilla-Torres, C.P., Cruz-Gonzalez, I., Gonzalez-Serrano, J.I., Beyoro-Amado, Z., Torres-Rios, G., Gonzalez-Otero, M., Cepa, J., González-Serrano, J. Ignacio, Bongiovanni, Ángel, Cedrés, Bernabé, Rodriguez, M.I., Lara-Lopez, M.A., Pović, Mirjana, Povic, M., Mancillas, Brisa, Negrete, Castalia Alenka, Negrete, C.A., Castillo-Fraile, Manuel, Mancillas, B. +71 morecore +1 more sourceExploring Lenticular Galaxy Formation in Field Environments Using NewHorizon: Evidence for Counterrotating Gas Accretion as a Formation Channel
The Astrophysical JournalThe formation pathways of lenticular galaxies (S0s) in field environments remain a matter of debate. We utilize the cosmological hydrodynamic simulation, NewHorizon , to investigate the issue. We select two massive star formation quenched S0s as our main Seongbong Han, J. K. Jang, Emanuele Contini, Yohan Dubois, Seyoung Jeon, Sugata Kaviraj, Taysun Kimm, Katarina Kraljic, Sree Oh, Sébastien Peirani, Christophe Pichon, Sukyoung K. Yi +11 moredoaj +1 more sourceThe inside-out quenching of the MHONGOOSE galaxy NGC 1371 [PDF]
We present the deepest 21 cm spectral line and 1.4 GHz broad-band continuum observations of nearby early-type spiral galaxy NGC 1371 as part of the MeerKAT H i Observations of Nearby Galactic Objects: Observing Southern Emitters (MHONGOOSE) survey.Oosterloo, T. A., Healy, J., Veronese, S.; id_orcid, Morganti, R., Maccagni, F. M., Kleiner, D., de Blok, W. J.G., Fraternali, F.; id_orcid, S. Veronese, J. Healy, F. Fraternali, W. J. G. de Blok, F. M. Maccagni, R. Morganti, T. A. Oosterloo, D. Kleiner +15 morecore +1 more sourceThe Structure and Formation Histories of Low-mass Quiescent Galaxies in the A2744 Cluster Environment
The Astrophysical JournalLow-mass quiescent galaxies are thought to predominantly reside in overdense regions, as environmental effects are often invoked to explain their shutdown of star formation. These longer-timescale quenching mechanisms—such as interactions with hot gas in Sam E. Cutler, John R. Weaver, Katherine E. Whitaker, Jenny E. Greene, David J. Setton, Zach J. Webb, Ayesha Abdullah, Aubrey Medrano, Rachel Bezanson, Gabriel Brammer, Robert Feldmann, Lukas J. Furtak, Karl Glazebrook, Ivo Labbe, Joel Leja, Danilo Marchesini, Tim B. Miller, Ikki Mitsuhashi, Themiya Nanayakkara, Erica J. Nelson, Richard Pan, Sedona H. Price, Katherine A. Suess, Bingjie Wang +23 moredoaj +1 more sourceAGN Host Galaxy Properties and Mass Function
, 2016 Supermassive black hole growth, nuclear activity, and galaxy evolution have been found to be closely related. In the context of AGN-galaxy coevolution, I will discuss about the relation found between the host galaxy properties and the central BH and I ...Bongiorno, Angela, Bongiorno, Angela (5203153) +1 morecore +1 more sourceSearching within Galaxies for the Earliest Signs of Quenching With Spatially Resolved Star Formation Histories in UVCANDELS Galaxies at z < 0.3
The Astrophysical JournalUnderstanding the complicated processes that regulate star formation and cause a galaxy to become quiescent is key to our comprehension of galaxy evolution.Charlotte Olsen, Eric Gawiser, Charlotte Welker, Harry Teplitz, Kartheik Iyer, Xin Wang, Marc Rafelski, Rogier A. Windhorst, Anton Koekemoer, Anahita Alavi, Ben Sunnquist, Norman Grogin, Yicheng Guo, Christopher J. Conselice, L. Y. Aaron Yung, Kalina Nedkova, Bahram Mobasher, Ray A. Lucas, Vihang Mehta, Y. Sophia Dai, Jonathan P. Gardner +20 moredoaj +1 more sourceStar formation and quenching in galaxy formation models [PDF]
, 2019 Galaxies locally have been observed to have a bimodal distribution for many properties, such as colour, star formation rate and morphology. These properties can be used to separate galaxies into two classes - the 'blue cloud' and the 'red sequence ...Asquith, Rachelcore Resolved Maps of Gas and Dust in a Massive Quiescent Galaxy at z = 2 from INQUEST-JWST: Evidence of Accretion and Rejuvenation
The Astrophysical JournalQuiescent galaxies in the distant Universe exhibit a range of gas content that may indicate a variety of quenching processes are at play. Mapping the distribution and kinematics of the gas can illuminate its origins, but nearly all such observations have Sai Gangula, Andrew B. Newman, Meng Gu, Sirio Belli, Katherine E. Whitaker, Tania M. Barone, Aliza Beverage, Andrea Bolamperti, Letizia Bugiani, Richard S. Ellis, Mariska Kriek, Allison Matthews, Themiya Nanayakkara +12 moredoaj +1 more source