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101
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102
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103
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104
Common-envelope evolution and stellar mergers
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 -
105
The nuclear stellar cluster in NGC 1068
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 -
106
Stellar populations in brightest cluster galaxies
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 -
107
Hydrogen-poor superluminous stellar explosions.
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 -
108
The evolution of the stellar hosts of radio galaxies
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 -
109
The nuclear stellar cluster in NGC 1068
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 -
110
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111
Gas and stellar kinematics in NGC 6240
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 -
112
Disk heating and stellar migration in galaxies
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 -
113
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114
Stellar populations in the SAMI Galaxy Survey
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 -
115
Stellar populations in KDCs of Sa galaxies
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 -
116
Modelling the Milky Way stellar halo
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 -
117
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118
On the formation of dwarf galaxies and stellar haloes
Published 2006“…We show that this gives a metallicity and total stellar mass consistent with the MW old stellar halo. © 2006 RAS.…”
Journal article -
119
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120
Flow damping in stellarators close to quasisymmetry
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