Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Rose, Marvin"'
Autor:
Pierce, Jonathon C. S., Tadhunter, Clive N., Almeida, Cristina Ramos, Bessiere, Patricia, Rose, Marvin
Radio AGNs with intermediate radio powers are capable of driving multi-phase outflows in galaxy bulges, and are also more common than their high-radio-power counterparts. In-depth characterisation of the typical host galaxies and likely triggering me
Externí odkaz:
http://arxiv.org/abs/1905.01315
Autor:
Rose, Marvin, Tadhunter, Clive, Almeida, Cristina Ramos, Zaurin, Javier Rodriguez, Santoro, Francesco, Spence, Robert
Although now routinely incorporated into hydrodynamic simulations of galaxy evolution, the true importance of the feedback effect of the outflows driven by active galactic nuclei (AGN) remains uncertain from an observational perspective. This is due
Externí odkaz:
http://arxiv.org/abs/1710.06600
We present a model for the classification of Coronal-Line Forest Active Galactic Nuclei (CLiF AGN). CLiF AGN are of special interest due to their remarkably large number of emission lines, especially forbidden high ionization lines (FHILs). Rose et a
Externí odkaz:
http://arxiv.org/abs/1604.04624
Autor:
Rose, Marvin
A key result of the Two Micron All Sky Survey (2MASS) was the discovery of a popula tion of AGN that appear redder than their traditional UV/optical selected counterparts at IR wavelengths. In order to investigate the nature of 2MASSselected AGN,
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.589142
Autor:
Faherty, Jacqueline K., Alatalo, K., Anderson, L. D., Assef, Roberto J., Gagliuffi, Daniella C. Bardalez, Barry, Megan, Benford, Dominic J., Bilicki, Maciej, Burningham, Ben, Christian, Damian J., Cushing, Michael C., Eisenhardt, Peter R., Elvisx, Martin, Fajardo-Acosta, S. B., Finkbeiner, Douglas P., Fischer, William J., Forrest, William J., Fowler, John, Gardner, Jonathan P., Gelino, Christopher R., Gorjian, V, Grillmair, Carl J., Gromadzki, Mariusz, Hall, Kendall P., Ivezi'c, Zeljko, Izumi, Natsuko, Kirkpatrick, J. Davy, Kovács, András, Lang, Dustin, Leisawitz, David, Liu, Fengchuan, Mainzer, A., Malek, Katarzyna, Marton, Gábor, Masci, Frank J., McLean, Ian S., Meisner, Aaron, Nikutta, Robert, Padgett, Deborah L., Patel, Rahul, Rebull, L. M., Rich, J. A., Ringwald, Frederick A., Rose, Marvin, Schneider, Adam C., Stassun, Keivan G, Stern, Daniel, Tsai, Chao-Wei, Wang, Feige, Weston, Madalyn E., L., Edward, Wright, Wu, Jingwen, Yang, Jinyi
During the "WISE at 5: Legacy and Prospects" conference in Pasadena, CA -- which ran from February 10 - 12, 2015 -- attendees were invited to engage in an interactive session exploring the future uses of the Wide-field Infrared Survey Explorer (WISE)
Externí odkaz:
http://arxiv.org/abs/1505.01923
Coronal-Line Forest Active Galactic Nuclei (CLiF AGN) are remarkable in the sense that they have a rich spectrum of dozens of coronal emission lines (e.g. [FeVII], [FeX] and [NeV]) in their spectra. Rose, Elvis & Tadhunter (2015) suggest that the inn
Externí odkaz:
http://arxiv.org/abs/1504.01663
We introduce Coronal-Line Forest Active Galactic Nuclei (CLiF AGN), AGN which have a rich spectrum of forbidden high-ionization lines (FHILs, e.g. [FeVII], [FeX] and [NeV]), as well as relatively strong narrow ($\sim$300 km s$^{-1}$) H$\alpha$ emissi
Externí odkaz:
http://arxiv.org/abs/1501.02705
On the nature of the red, 2MASS selected AGN in the local Universe I: an optical spectroscopic study
We present optical spectra for a representative sample of 27 nearby (z < 0.2) 2MASS-selected AGN with red near-IR colours (J-K 2.0). The spectra were taken with the ISIS spectrograph on the WHT with the aim of determining the nature of the red 2MASS
Externí odkaz:
http://arxiv.org/abs/1303.7112
Mergers and interactions in SDSS type 2 quasars at z~0.3-0.4. SDSS J143027.66-005614.8: a case study
Autor:
Villar-Martin, Montse, Cabrera-Lavers, Antonio, Bessiere, Patricia, Tadhunter, Clive, Rose, Marvin, de Breuck, Carlos
We present a compilation of HST images of 58 luminous SDSS type 2 AGNs at 0.3
Externí odkaz:
http://arxiv.org/abs/1202.1729
We present spectroscopic observations of the type 2 quasar SDSS J11311.05+162739.5 (Q1131+16 hereafter; z=0.1732), which has the richest spectrum of forbidden high ionisation lines (FHIL, e.g. [Fe \textsc{vii}], [Fe \textsc{x}], [Fe \textsc{xi}] and
Externí odkaz:
http://arxiv.org/abs/1103.0660