Zobrazeno 1 - 10
of 232
pro vyhledávání: '"A, Chadayammuri"'
Autor:
Chadayammuri, Urmila, Eisert, Lukas, Pillepich, Annalisa, Lehle, Katrin, Ayromlou, Mohammadreza, Nelson, Dylan
The physical properties of the intracluster medium (ICM) reflect signatures of the underlying gravitational potential, mergers and strong interactions with other halos and satellite galaxies, as well as galactic feedback from supernovae and supermass
Externí odkaz:
http://arxiv.org/abs/2410.22416
Autor:
Fouesneau, Morgan, Momcheva, Ivelina G., Chadayammuri, Urmila, Demianenko, Mariia, Dumont, Antoine, Hviding, Raphael E., Kahle, K. Angelique, Pulatova, Nadiia, Rajpoot, Bhavesh, Scheuck, Marten B., Seeburger, Rhys, Semenov, Dmitry, Villaseñor, Jaime I.
ChatGPT and other state-of-the-art large language models (LLMs) are rapidly transforming multiple fields, offering powerful tools for a wide range of applications. These models, commonly trained on vast datasets, exhibit human-like text generation ca
Externí odkaz:
http://arxiv.org/abs/2409.20252
Abell 2744, also known as Pandora's Cluster, is a complex merging galaxy cluster. While a major merger is clear along the north-south axis, the dynamical state of the northwest subcluster has been highly uncertain. We present ultra-deep ($\approx$2.1
Externí odkaz:
http://arxiv.org/abs/2407.03142
Although supermassive black holes (SMBHs) reside in the heart of virtually every massive galaxy, it remains debated whether dwarf galaxies also commonly host SMBHs. Because low-mass galaxies may retain a memory of the assembly history of their black
Externí odkaz:
http://arxiv.org/abs/2406.01707
Autor:
Silich, Emily M., Bellomi, Elena, Sayers, Jack, ZuHone, John, Chadayammuri, Urmila, Golwala, Sunil, Hughes, David, Montaña, Alfredo, Mroczkowski, Tony, Nagai, Daisuke, Sánchez, David, Stanford, S. A., Wilson, Grant, Zemcov, Michael, Zitrin, Adi
Galaxy cluster mergers are representative of a wide range of physics, making them an excellent probe of the properties of dark matter and the ionized plasma of the intracluster medium. To date, most studies have focused on mergers occurring in the pl
Externí odkaz:
http://arxiv.org/abs/2404.04379
Autor:
Kovacs, Orsolya E., Bogdan, Akos, Natarajan, Priyamvada, Werner, Norbert, Azadi, Mojegan, Volonteri, Marta, Tremblay, Grant R., Chadayammuri, Urmila, Forman, William R., Jones, Christine, Kraft, Ralph P.
While supermassive black holes (BHs) are widely observed in the nearby and distant universe, their origin remains debated with two viable formation scenarios with light and heavy seeds. In the light seeding model, the first BHs form from the collapse
Externí odkaz:
http://arxiv.org/abs/2403.14745
Autor:
Felix, Sharon, Gogoi, Antareep, Shavelle, Kaitlyn, Sike, Brandon, King, Lindsay, Andreon, Stefano, Chadayammuri, Urmila, ZuHone, John, Romero, Charles
JKCS041 ($z=1.8$) is one of the most distant galaxy cluster systems known, seen when the Universe was less than 4 billion years old. Recent Sunyaev-Zeldovich (SZ) observations show a temperature decrement that is less than expected based on mass esti
Externí odkaz:
http://arxiv.org/abs/2402.13334
Autor:
Richard-Laferrière, A., Russell, H. R., Fabian, A. C., Chadayammuri, U., Reynolds, C. S., Canning, R. E. A., Edge, A. C., Hlavacek-Larrondo, J., King, L. J., McNamara, B. R., Nulsen, P. E. J., Sanders, J. S.
The cluster of galaxies Abell 2146 is undergoing a major merger and is an ideal cluster to study ICM physics, as it has a simple geometry with the merger axis in the plane of the sky, its distance allows us to resolve features across the relevant sca
Externí odkaz:
http://arxiv.org/abs/2310.11491
Autor:
Silich, Emily M., Bellomi, Elena, Sayers, Jack, ZuHone, John, Chadayammuri, Urmila, Golwala, Sunil, Hughes, David, Montaña, Alfredo, Mroczkowski, Tony, Nagai, Daisuke, Sánchez, David, Stanford, S. A., Wilson, Grant, Zemcov, Michael, Zitrin, Adi
Galaxy cluster mergers are rich sources of information to test cluster astrophysics and cosmology. However, cluster mergers produce complex projected signals that are difficult to interpret physically from individual observational probes. Multi-probe
Externí odkaz:
http://arxiv.org/abs/2309.12533
Galaxy cluster mass functions are a function of cosmology, but mass is not a direct observable, and systematic errors abound in all its observable proxies. Mass-free inference can bypass this challenge, but it requires large suites of simulations spa
Externí odkaz:
http://arxiv.org/abs/2307.16733