Showing 101 - 120 results of 5,521 for search '"Stellarator"', query time: 0.11s Refine Results
  1. 101
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  4. 104

    Common-envelope evolution and stellar mergers by Podsiadlowski, P

    Published 2001
    “…In this case, it is possible that a CE system (contact system) may become semi-detached again without experiencing significant spiral-in, and the mass loss from the contact configuration is best described by a frictionally driven stellar wind. If the spiralling-in star is compact, CE ejection may also occur when it penetrates below the convective envelope. …”
    Conference item
  5. 105

    The nuclear stellar cluster in NGC 1068 by Thatte, N, Genzel, R, Kroker, H, Krabbe, A, TacconiGarman, L, Maiolino, R, Tecza, M

    Published 1997
    “…We present new near-infrared integral field spectroscopy and adaptive optics imaging of the nucleus of NGC 1068. Using the stellar CO absorption features in the H and K bands, we have identified a moderately extincted stellar core centered on the nuclear position and of intrinsic size similar to 50 pc. …”
    Conference item
  6. 106

    Stellar populations in brightest cluster galaxies by Loubser, S, Sanchez-Blazquez, P, Soechting, I, Sansom, A

    Published 2010
    “…We present the results of an investigation of a large sample of brightest cluster galaxies (BCGs), their kinematic and stellar population properties and the relationships between these and the properties of the host clusters. …”
    Conference item
  7. 107

    Hydrogen-poor superluminous stellar explosions. by Quimby, R, Kulkarni, SR, Kasliwal, M, Gal-Yam, A, Arcavi, I, Sullivan, M, Nugent, P, Thomas, R, Howell, D, Nakar, E, Bildsten, L, Theissen, C, Law, N, Dekany, R, Rahmer, G, Hale, D, Smith, R, Ofek, E, Zolkower, J, Velur, V, Walters, R, Henning, J, Bui, K, McKenna, D, Poznanski, D

    Published 2011
    “…Supernovae are stellar explosions driven by gravitational or thermonuclear energy that is observed as electromagnetic radiation emitted over weeks or more. …”
    Journal article
  8. 108

    The evolution of the stellar hosts of radio galaxies by Lacy, M, Bunker, A, Ridgway, SE

    Published 2000
    “…The hosts brighten significantly with redshift, consistent with the passive evolution of a stellar population that formed at z ≳ 3. This scenario is consistent with studies of host galaxy morphology and submillimeter continuum emission, both of which show strong evolution at z ≳ 2.5. …”
    Journal article
  9. 109

    The nuclear stellar cluster in NGC 1068 by Thatte, N, Genzel, R, Tacconi, L, Krabbe, A, Kroker, H

    Published 1997
    “…We have imaged a compact stellar cluster, with a characteristic size of 50 pc, toward the nucleus of NGC 1068, using near IR imaging spectroscopy of stellar absorption features in the H and K bands. …”
    Conference item
  10. 110
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    Gas and stellar kinematics in NGC 6240 by Tecza, M, Tacconi, L, Genzel, R

    Published 2001
    “…We present results from sub-arcsecond near infrared integral field spectroscopy and millimeter IRAM-interferometry of the interacting galaxy NGC 6240. Using stellar absorption features in the NIR we determined the stellar velocity field and dispersion in NGC 6240. …”
    Conference item
  12. 112

    Disk heating and stellar migration in galaxies by Binney, J, Sellwood, J

    Published 2000
    “…The paper claimed that significant radial migration of stars in a stellar disk like that of the Milky Way could not occur. …”
    Journal article
  13. 113
  14. 114

    Stellar populations in the SAMI Galaxy Survey by Watson, PJ

    Published 2023
    “…We apply this method to galaxies drawn from the SAMI Galaxy Survey, deriving seeing-corrected radial stellar population gradients for 1453 galaxies. On average, galaxies in our sample have flat age and [α/Fe] gradients, but negative metallicity gradients. …”
    Thesis
  15. 115

    Stellar populations in KDCs of Sa galaxies by Falcn-Barroso, J, Bacon, R, Cappellari, M, Davies, R, De Zeeuw, P, Emsellem, E, Krajnović, D, Kuntschner, H, McDermid, R, Peletier, R, Sarzi, M, Van De Ven, G

    Published 2006
    “…We show how the V/ maps can be used to highlight the presence of the KDC and investigate their stellar populations (i.e. age) to understand their origin (i.e. secular vs hierarchical scenarios). …”
    Journal article
  16. 116

    Modelling the Milky Way stellar halo by Fermani, F

    Published 2013
    “…<p>We motivate the importance of understanding the kinematics and dynamics of the Milky Way stellar halo both in unravelling the formation history and evolution of our host Galaxy and in the more general context of galaxy dynamics.…”
    Thesis
  17. 117
  18. 118

    On the formation of dwarf galaxies and stellar haloes by Read, J, Pontzen, A, Viel, M

    Published 2006
    “…We show that this gives a metallicity and total stellar mass consistent with the MW old stellar halo. © 2006 RAS.…”
    Journal article
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    Flow damping in stellarators close to quasisymmetry by Calvo, I, Parra, F, Velasco, J, Alonso, J

    Published 2014
    “…Quasisymmetric stellarators are a type of optimized stellarators for which flows are undamped to lowest order in an expansion in the normalized Larmor radius. …”
    Journal article