Now showing items 161-170 of 70554

    • Chong, Jane ; Gagné, M.; Dunlop, Patrick ; Wee, S. (2024)
      Despite the importance of employee work motivation in organizations, little is known about how newcomers develop high-quality motivation to function optimally at work. We propose internalization — a process whereby newcomers ...
    • Gagne, Marylene ; Agate, Daniel (2024)
      In July of 2024, our research team held “roundtable” discussions with 40 industry representatives from Australia, Canada, Europe, and the United States to better understand the organisational design issues present in ...
    • Holoien, T.W.S.; Auchettl, K.; Tucker, M.A.; Shappee, B.J.; Patel, S.G.; Miller-Jones, James ; Mockler, B.; Groenewald, D.L.N.; Hinkle, J.T.; Brown, J.S.; Kochanek, C.S.; Stanek, K.Z.; Chen, P.; Dong, S.; Prieto, J.L.; Thompson, T.A.; Beaton, R.L.; Connor, T.; Cowperthwaite, P.S.; Dahmen, L.; French, K.D.; Morrell, N.; Buckley, D.A.H.; Gromadzki, M.; Roy, R.; Coulter, D.A.; Dimitriadis, G.; Foley, R.J.; Kilpatrick, C.D.; Piro, A.L.; Rojas-Bravo, C.; Siebert, M.R.; Velzen, S.V. (2020)
      We present nearly 500 days of observations of the tidal disruption event (TDE) ASASSN-18pg, spanning from 54 days before peak light to 441 days after peak light. Our data set includes X-ray, UV, and optical photometry, ...
    • Soria, Roberto ; Pakull, M.W.; Motch, C.; Miller-Jones, James ; Schwope, A.D.; Urquhart, R.T.; Ryan, M.S. (2021)
      Some ultraluminous X-ray sources (ULXs) are surrounded by collisionally ionized bubbles, larger and more energetic than supernova remnants: they are evidence of the powerful outflows associated with super-Eddington X-ray ...
    • Soria, Roberto ; Kolehmainen, M.; Graham, A.W.; Swartz, D.A.; Yukita, M.; Motch, C.; Jarrett, T.H.; Miller-Jones, James ; Plotkin, Richard ; MacCarone, T.J.; Ferrarese, L.; Guest, A.; Lançon, A. (2022)
      We present an analysis of the ultraluminous X-ray source (ULX) population in 75 Virgo cluster late-Type galaxies, including all those with a star formation rate 1 M yr-1 and a representative sample of the less star forming ...
    • Yao, Y.; Lu, W.; Guolo, M.; Pasham, D.R.; Gezari, S.; Gilfanov, M.; Gendreau, K.C.; Harrison, F.; Cenko, S.B.; Kulkarni, S.R.; Miller, J.M.; Walton, D.J.; García, J.A.; Velzen, S.V.; Alexander, K.D.; Miller-Jones, James ; Nicholl, M.; Hammerstein, E.; Medvedev, P.; Stern, D.; Ravi, V.; Sunyaev, R.; Bloom, J.S.; Graham, M.J.; Kool, E.C.; Mahabal, A.A.; Masci, F.J.; Purdum, J.; Rusholme, B.; Sharma, Y.; Smith, R.; Sollerman, J. (2022)
      We present X-ray, UV, optical, and radio observations of the nearby (≈78 Mpc) tidal disruption event AT2021ehb/ZTF21aanxhjv during its first 430 days of evolution. AT2021ehb occurs in the nucleus of a galaxy hosting a≈107 ...
    • Malyali, A.; Liu, Z.; Rau, A.; Grotova, I.; Merloni, A.; Goodwin, Adelle ; Anderson, Gemma ; Miller-Jones, James ; Kawka, A.; Arcodia, R.; Buchner, J.; Nandra, K.; Homan, D.; Krumpe, M. (2023)
      The ROSAT-selected tidal disruption event (TDE) candidate RX J133157.6-324319.7 (J1331), was detected in 1993 as a bright (0.2-2 keV flux of $(1.0 \pm 0.1) \times 10^{-12}$ erg s$^{-1}$ cm$^{-2}$), ultra-soft ($kT=0.11 \pm ...
    • Beuchert, T.; Middleton, M.J.; Soria, R.; Miller-Jones, James ; Dauser, T.; Roberts, T.P.; Sathyaprakash, R.; Markoff, S. (2024)
      In order to understand the nature of super-Eddington accretion we must explore both the emission emerging directly from the inflow and its impact on the surroundings. In this paper, we test whether we can use the optical ...
    • Christy, C.T.; Alexander, K.D.; Margutti, R.; Wieringa, M.; Cendes, Y.; Chornock, R.; Laskar, T.; Berger, E.; Bietenholz, M.; Coppejans, D.L.; De Colle, F.; Eftekhari, T.; Holoien, T.W.S.; Matsumoto, T.; Miller-Jones, James ; Ramirez-Ruiz, E.; Saxton, R.; van Velzen, S. (2024)
      We present detailed radio observations of the tidal disruption event (TDE) ASASSN-19bt/AT 2019ahk, obtained with the Australia Telescope Compact Array, the Atacama Large Millimeter/submillimeter Array, and the MeerKAT ...
    • Panurach, T.; Dage, Kristen ; Urquhart, R.; Plotkin, R.M.; Paul, J.D.; Bahramian, Arash ; Brumback, M.C.; Galvin, Tim ; Molina, I.; Miller-Jones, James ; Saikia, P. (2024)
      Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve as potential candidates for (sub-Eddington) ...