Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Nyland, Kristina"'
Autor:
Morganti, Raffaella, Schulz, Robert, Nyland, Kristina, Paragi, Zsolt, Oosterloo, Tom, Mahony, Elizabeth, Murthy, Suma, Lago, M.T.
Publikováno v:
Astronomy in Focus-XXX: Molecular versus excitonic disorder inindividual artificial light-harvesting systems, 30, 74-77
Radio jets can play multiple roles in the feedback loop by regulating the accretion of the gas, by enhancing gas turbulence, and by driving gas outflows. Numerical simulations are beginning to make detailed predictions about these processes. Using hi
Autor:
Emonts, Bjorn, Lacy, Mark, Nyland, Kristina, Mason, Brian, Lehnert, Matthew, Carilli, Chris, Sarazin, Craig, Cai, Zheng, Chatterjee, Suchetana, Dannerbauer, Helmut, Gallagher, John, Harrington, Kevin, Naryanan, Desika, Riechers, Dominik, Rocha, Graca
Massive galaxies at high-z are known to co-evolve with their circumgalactic medium (CGM). If we want to truly understand the role of the CGM in the early evolution of galaxies and galaxy-clusters, we need to fully explore the multi-phase nature of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_______::476e8ddec782ec57166ae91162c7baaf
http://arxiv.org/abs/1905.05808
http://arxiv.org/abs/1905.05808
Autor:
Mroczkowski, Tony, Nagai, Daisuke, Andreani, Paola, Arnaud, Monique, Bartlett, James, Battaglia, Nicholas, Basu, Kaustuv, Bulbul, Esra, Chluba, Jens, Churazov, Eugene, CICONE, CLAUDIA, Crites, Abigail, Devlin, Mark, DeNigris, Nat, Dicker, Simon, DI MASCOLO, LUCA, GASPARI, MASSIMO, Golwala, Sunil, Guglielmetti, Fabrizia, Hill, J. Colin, Kitayama, Tetsu, Klaassen, Pamela, Kohno, Kotaro, Komatsu, Eiichiro, Kneissl, Ruediger, Lacy, Mark, Mason, Brian, Nyland, Kristina, Romero, Charles, Sayers, Jack, Sehgal, Neelima, Simon, Sara, Sunyaev, Rashid, Wilson, Grant, Zemcov, Michael, ZuHone, John
The Sunyaev-Zeldovich (SZ) effect was first predicted nearly five decades ago, but has only recently become a mature tool for performing high resolution studies of the warm and hot ionized gas in and between galaxies, groups, and clusters. Galaxy gro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9d0b18c0d00c666fa4d18fa19b39e46
http://arxiv.org/abs/1903.02595
http://arxiv.org/abs/1903.02595
Autor:
Perlman, Eric S., Birkinshaw, Mark, Kadler, Matthias, Komissarov, Serguei, Lister, Matthew, Meier, David, Meyer, Eileen, Nakamura, Masanori, Nyland, Kristina, ODea, Christopher, Worrall, Diana, Zdziarski, Andrzej
Jets are a ubiquitous part of the accretion process, seen in a wide variety of objects ranging from active galaxies (AGN) to X-ray binary stars and even newly formed stars. AGN jets are accelerated by the supermassive black hole of their host galaxy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa58bb51843b0350c6371ccf614b0820
Autor:
Emonts, Bjorn, Lacy, Mark, Nyland, Kristina, Mason, Brian, Lehnert, Matthew, Carilli, Chris, Sarazin, Craig, Cai, Zheng, Chatterjee, Suchetana, Dannerbauer, Helmut, Gallagher, John, Harrington, Kevin, Naryanan, Desika, Riechers, Dominik, Rocha, Graca
Massive galaxies at high-z are known to co-evolve with their circumgalactic medium (CGM). If we want to truly understand the role of the CGM in the early evolution of galaxies and galaxy-clusters, we need to fully explore the multi-phase nature of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::035bc7d8e8832e60585192fab6945f56
Autor:
Wrobel, Joan M., Haiman, Zoltan, Holley-Bockelmann, Kelly, Inayoshi, Kohei, Lazio, Joe, Maccarone, Tom, Miller-Jones, James, Nyland, Kristina, Plotkin, Rich
Intermediate-mass black holes (IMBHs) have masses of about 100 to 100,000 solar masses. They remain elusive. Observing IMBHs in present-day globular clusters (GCs) would validate a formation channel for seed black holes in the early universe and info
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebfe810d614309bcdcc54f07bdcbed37
Autor:
Morganti, Raffaella, Schulz, Robert, Nyland, Kristina, Paragi, Zsolt, Oosterloo, Tom, Mahony, Elizabeth, Murthy, Suma
Radio jets can play multiple roles in the feedback loop by regulating the accretion of the gas, by enhancing gas turbulence, and by driving gas outflows. Numerical simulations are beginning to make detailed predictions about these processes. Using hi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aba0961f9aa0b2fb30a4d3e3c252f75b
Autor:
Nyland, Kristina, Kirkpatrick, Allison, Spilker, Justin, Boizelle, Benjamin, Hall, Kirsten R., MUKHERJEE, DIPANJAN, Patil, Pallavi, Lacy, Mark, PRANDONI, ISABELLA, Rujopakarn, Wiphu, Harwood, Jeremy, Kimball, Amy, Alatalo, Katherine, Clarke, Tracy
A key missing element in our understanding of cosmic assembly is the nature of energetic feedback from supermassive black holes (SMHBs) and the impact of active galactic nuclei (AGN) on galaxy evolution. The next-generation Very Large Array (ngVLA),
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4759::7f5d9a781a1a3346af43171038910944
http://hdl.handle.net/20.500.12386/32446
http://hdl.handle.net/20.500.12386/32446
Autor:
Greene, Jenny E, Barth, Aaron, Bellini, Andrea, Bellovary, Jillian, Holley-Bockelmann, Kelly, Do, Tuan, Gallo, Elena, Gebhardt, Karl, Gultekin, Kayhan, Haiman, Zoltan, Hosek, Matthew, Kim, Dongwon, Libralato, Mattia, Lu, Jessica, Nyland, Kristina, Malkan, Matthew, Reines, Amy, Seth, Anil, Treu, Tommaso, Walsh, Jonelle, Wrobel, Joan
We have compelling evidence for stellar-mass black holes (BHs) of ~5-80 M_sun that form through the death of massive stars. We also have compelling evidence for so-called supermassive BHs (10^5-10^10 M_sun) that are predominantly found in the centers
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d93b40e564aef8041fe9d13970fccf2
Most of the stars today reside in galactic spheroids, whose properties are tightly tied to the supermassive black holes (MBHs) at their centers, implying that the accretion activity onto MBHs leaves a lasting imprint on the evolution of their host ga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d237e496d60d2c97200d16772276ae5
http://arxiv.org/abs/1810.07098
http://arxiv.org/abs/1810.07098