Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Nyland, K. E."'
Autor:
Willner, S. P., Gim, H. B., Polletta, M. del Carmen, Cohen, S. H., Willmer, C. N. A., Zhao, X., D'Silva, J. C. J., Jansen, R. A., Koekemoer, A. M., Summers, J., Windhorst, R. A., Coe, D., Conselice, C. J., Driver, S. P., Frye, B., Grogin, N. A., Marshall, M. A., Nonino, M., Ortiz III, R., Pirzkal, N., Robotham, A., Rutkowski, M. J., Ryan, Jr., R. E., Tompkins, S., Yan, H., Hammel, H. B., Milam, S. N., Adams, N. J., Beacom, J. F., Bhatawdekar, R., Cheng, C., Civano, F., Cotton, W., Hyun, M., Kikuta, S., Nyland, K. E., Peters, W. M., Petric, A., Röttgering, H. J. A., Shimwell, T., Yun, M. S.
The Time Domain Field (TDF) near the North Ecliptic Pole in JWST's continuous-viewing zone will become a premier "blank field" for extragalactic science. JWST/NIRCam data in a 16 arcmin$^2$ portion of the TDF identify 4.4 $\mu$m counterparts for 62 o
Externí odkaz:
http://arxiv.org/abs/2309.13008
Intermediate-mass black holes (IMBHs) by definition have masses of $M_{\rm IMBH} \sim 10^{2-5}~M_\odot$, a range with few observational constraints. Finding IMBHs in globular star clusters (GCs) would validate a formation channel for massive black-ho
Externí odkaz:
http://arxiv.org/abs/2106.13862
Autor:
Wrobel, J. M., Nyland, K. E.
The NSF's Karl G.\ Jansky Very Large Array (VLA) was used at 3~cm to search for accretion signatures from intermediate-mass black holes (IMBHs) in 19 globular star clusters (GCs) in NGC\,3115, an early-type galaxy at a distance of 9.4 Mpc. The 19 hav
Externí odkaz:
http://arxiv.org/abs/2007.12093
Using the Next Generation Very Large Array (ngVLA), we will make a comprehensive inventory of intermediate-mass black holes (IMBHs) in hundreds of globular cluster systems out to a distance of 25 Mpc. IMBHs have masses of about 100 to 100,000 solar m
Externí odkaz:
http://arxiv.org/abs/1806.06052
Forbes et al. recently used the Hubble Space Telescope to localize hundreds of candidate star clusters in NGC 1023, an early-type galaxy at a distance of 11.1 Mpc. Old stars dominate the light of 92% of the clusters and intermediate-age stars dominat
Externí odkaz:
http://arxiv.org/abs/1507.07613
Akademický článek
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Autor:
Alatalo, K., Nyland, K. E., Graves, G., Deustua, S., Young, L. M., Davis, T. A., Bureau, M., Bayet, E., Blitz, L., Bois, M., Bournaud, F., Cappellari, M., Davies, R. L., de Zeeuw, P. T., Emsellem, E., Khochfar, S., Krajnovic, D., Kuntschner, H., McDermid, R. M., Morganti, R., Naab, T., Oosterloo, T., Sarzi, M., Scott, N., Serra, P., Weijmans, A.
We detail the rich molecular story of NGC 1266, its serendipitous discovery within the ATLAS3D survey (Cappellari et al. 2011) and how it plays host to an AGN-driven molecular outflow, potentially quenching all of its star formation (SF) within the n
Externí odkaz:
http://arxiv.org/abs/1211.3441
Autor:
Alatalo, K., Nyland, K. E., Graves, G., Deustua, S., Wrobel, J., Young, L. M., Davis, T. A., Bureau, M., Bayet, E., Blitz, L., Bois, M., Bournaud, F., Cappellari, M., Davies, R. L., de Zeeuw, P. T., Emsellem, E., Khochfar, S., Krajnovic, D., Kuntschner, H., Martin, S., McDermid, R. M., Morganti, R., Naab, T., Oosterloo, T., Sarzi, M., Scott, N., Serra, P., Weijmans, A.
NGC 1266 is a nearby field galaxy observed as part of the ATLAS3D survey (Cappellari et al. 2011). NGC 1266 has been shown to host a compact (< 200 pc) molecular disk and a mass-loaded molecular outflow driven by the AGN (Alatalo et al. 2011). Very L
Externí odkaz:
http://arxiv.org/abs/1211.3438
Autor:
Druckenmiller, Matthew L., Moon, Twila A., Thoman, Richard L., Ballinger, Thomas J., Berner, Logan T., Bernhard, Germar H., Bhatt, Uma S., Bjerke, Jarle W., Box, Jason E., Brown, R., Cappelen, John, Christiansen, Hanne H., Decharme, B., Derksen, C., Divine, Dmitry, Drozdov, D. S., Elias Chereque, A., Epstein, Howard E., Farquharson, L. M., Farrell, Sinead L., Fausto, Robert S., Fettweis, Xavier, Fioletov, Vitali E., Forbes, Bruce C., Frost, Gerald V., Gargulinski, Emily, Gerland, Sebastian, Goetz, Scott J., Grabinski, Z., Grooß, Jens-Uwe, Haas, Christian, Hanna, Edward, Hanssen-Bauer, Inger, Hendricks, Stefan, Holmes, Robert M., Ialongo, Iolanda, Isaksen, K., Jain, Piyush, Johnsen, Bjørn, Kaleschke, L., Kholodov, A. L., Kim, Seong-Joong, Korsgaard, Niels J., Labe, Zachary, Lakkala, Kaisa, Lara, Mark J., Loomis, Bryant, Luojus, K., Macander, Matthew J., Malkova, G. V., Mankoff, Kenneth D., Manney, Gloria L., McClelland, James W., Meier, Walter N., Mote, Thomas, Mudryk, L., Müller, Rolf, Nyland, K. E., Overland, James E., Park, T., Pavlova, Olga, Perovich, Don, Petty, Alek, Phoenix, Gareth K., Raynolds, Martha K., Reijmer, C. H., Richter-Menge, Jacqueline, Ricker, Robert, Romanovsky, Vladimir E., Scott, Lindsay, Shapiro, Hazel, Shiklomanov, Alexander I., Shiklomanov, Nikolai I., Smeets, C. J. P. P., Smith, Sharon L., Soja, Amber, Spencer, Robert G. M., Starkweather, Sandy, Streletskiy, Dimitri A., Suslova, Anya, Svendby, Tove, Tank, Suzanne E., Tedesco, Marco, Tian-Kunze, X., Timmermans, Mary-Louise, Tømmervik, Hans, Tretiakov, Mikhail, Tschudi, Mark, Vakhutinsky, Sofia, van As, Dirk, van de Wal, R. S. W., Veraverbeke, Sander, Walker, Donald A., Walsh, John E., Wang, Muyin, Webster, Melinda, Winton, Øyvind, Wood, K., York, Alison, Ziel, Robert, Sub Dynamics Meteorology, Proceskunde, Sub Algemeen Marine & Atmospheric Res, Marine and Atmospheric Research
Publikováno v:
Bulletin of the American Meteorological Society
Bulletin of the American Meteorological Society, American Meteorological Society, 2021, 102 (8), pp.S263-S316. ⟨10.1175/BAMS-D-21-0086.1⟩
Bulletin of the American Meteorological Society, 102(8), S263. American Meteorological Society
Bulletin of the American Meteorological Society, 2021, 102 (8), pp.S263-S316. ⟨10.1175/BAMS-D-21-0086.1⟩
Bulletin of the American Meteorological Society, American Meteorological Society, 2021, 102 (8), pp.S263-S316. ⟨10.1175/BAMS-D-21-0086.1⟩
Bulletin of the American Meteorological Society, 102(8), S263. American Meteorological Society
Bulletin of the American Meteorological Society, 2021, 102 (8), pp.S263-S316. ⟨10.1175/BAMS-D-21-0086.1⟩
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7f8ee636e098239d0e739103d46845c
https://hal.archives-ouvertes.fr/hal-03403005
https://hal.archives-ouvertes.fr/hal-03403005
Autor:
Lazio, T. Joseph W., Alatalo, Katherine, Blecha, Laura, Boizelle, Benjamin, Bower, Geoffrey C., Braatz, James, Bogdanovic, Tamara, Brisken, Walter, Burke-Spolaor, Sarah, Carbone, Dario, Chomiuk, Laura, Civano, Francesca M., Comerford, Julia, Condon, James, Coppejans, Deanne, Corsi, Alessandra, Darling, Jeremiah K., Davis, Timothy A., Frail, Dale A., Hall, Kirsten R., Hallinan, Gregg, Harwood, Jeremy, Kharb, Preeti, Kimball, Amy, Kirkpatrick, Allison, Kording, E. G., Lacy, Mark, Lazzati, Davide, Lister, Matthew L., Liu, Xin, Maccarone, Thomas J., Metzger, Brian, Miller-Jones, J. C. A., MUKHERJEE, DIPANJAN, Nyland, K. E., O'Shaughnessy, Richard, Owen, Benjamin, Patil, Pallavi, Pesce, Dominic, Plotkin, Richard M., PRANDONI, ISABELLA, Ravi, Vikram, Reid, Mark, Reines, Amy, Rujopakarn, Wiphu, Rupen, Michael P., Sand, David, Shen, Yue, Simon, Joseph, Sivakoff, Gregory R., Strader, Jay, Taylor, Greg B., Taylor, Stephen, van Velzen, Sjoert
The next-generation Very Large Array (ngVLA) will be a powerful telescope for finding and studying black holes across the entire mass range. High-resolution imaging abilities will allow the separation of low-luminosity black holes in the local Univer
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4759::248c8c3f8c2cbf983f832435a4ebb6c9
http://hdl.handle.net/20.500.12386/32445
http://hdl.handle.net/20.500.12386/32445