Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Nyland, Kristina"'
Autor:
Schwartzman, Emma, Clarke, Tracy E., Nyland, Kristina, Secrest, Nathan J., Pfeifle, Ryan W., Schmitt, Henrique R., Satyapal, Shobita, Rothberg, Barry
Binary and dual active galactic nuclei (AGN) are an important observational tool for studying the formation and dynamical evolution of galaxies and supermassive black holes (SMBHs). An entirely new method for identifying possible AGN pairs makes use
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed881963f5e2bdaeac82df7949eb7a63
http://arxiv.org/abs/2306.13219
http://arxiv.org/abs/2306.13219
Autor:
Ni, Qingling, Brandt, W. N., Chen, Chien-Ting, Luo, Bin, Nyland, Kristina, Yang, Guang, Zou, Fan, Aird, James, Alexander, David M., Bauer, Franz Erik, Lacy, Mark, Lehmer, Bret D., Mallick, Labani, Salvato, Mara, Schneider, Donald P., Tozzi, Paolo, Traulsen, Iris, Vaccari, Mattia, Vignali, Cristian, Vito, Fabio, Xue, Yongquan, Banerji, Manda, Chow, Kate, Comastri, Andrea, Del Moro, Agnese, Gilli, Roberto, Mullaney, James, Paolillo, Maurizio, Schwope, Axel, Shemmer, Ohad, Sun, Mouyuan, Timlin, John D., III, Trump, Jonathan R.
Publikováno v:
Ni, Q, Brandt, W N, Chen, C, Luo, B, Nyland, K, Yang, G, Zou, F, Aird, J, Alexander, D M, Bauer, F E, Lacy, M, Lehmer, B D, Mallick, L, Salvato, M, Schneider, D P, Tozzi, P, Traulsen, I, Vaccari, M, Vignali, C, Vito, F, Xue, Y, Banerji, M, Chow, K, Comastri, A, Del Moro, A, Gilli, R, Mullaney, J, Paolillo, M, Schwope, A, Shemmer, O, Sun, M, Timlin III, J D & Trump, J R 2021, ' The XMM-SERVS survey: XMM-Newton point-source Catalogs for the W-CDF-S and ELAIS-S1 fields ', Astrophysical Journal Supplement, vol. 256, no. 1, 21 . https://doi.org/10.3847/1538-4365/ac0dc6
The Astrophysical Journal Supplement Series, 2021, Vol.256(1), pp.21 [Peer Reviewed Journal]
The Astrophysical Journal Supplement Series, 2021, Vol.256(1), pp.21 [Peer Reviewed Journal]
We present the X-ray point-source catalogs in two of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields, W-CDF-S (4.6 deg$^2$) and ELAIS-S1 (3.2 deg$^2$), aiming to fill the gap between deep pencil-beam X-ray surveys and sh
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:
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
The Next-Generation Very Large Array (ngVLA) will revolutionize our understanding of the Early Universe by tracing the coldest phase of molecular gas -the raw ingredient for star formation- in the most distant galaxies and galaxy-clusters. The km-sca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c55713acc826be3af1acbb8ad711eb61
http://arxiv.org/abs/1810.06770
http://arxiv.org/abs/1810.06770