Zobrazeno 1 - 9
of 9
pro vyhledávání: '"K E Harborne"'
Autor:
Caro Derkenne, Richard M McDermid, Adriano Poci, J Trevor Mendel, Francesco D’Eugenio, Seyoung Jeon, Rhea-Silvia Remus, Sabine Bellstedt, Andrew J Battisti, Joss Bland-Hawthorn, Anna Ferré-Mateu, Caroline Foster, K E Harborne, Claudia D P Lagos, Yingjie Peng, Piyush Sharda, Gauri Sharma, Sarah Sweet, Kim-Vy H Tran, Lucas M Valenzuela, Sam Vaughan, Emily Wisnioski, Sukyoung K Yi
We investigate the impact of environment on the internal mass distribution of galaxies using the Middle Ages Galaxy Properties with Integral field spectroscopy (MAGPI) survey. We use 2D resolved stellar kinematics to construct Jeans dynamical models
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9fcc36de10c9165e122f07cfc811688f
http://arxiv.org/abs/2306.09630
http://arxiv.org/abs/2306.09630
Autor:
Eric Emsellem, Ruby J. Wright, Thomas A. Davison, Caroline Foster, K. E. Harborne, Claudia del P. Lagos, Jesse van de Sande, Luca Cortese
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 509, pp.4372-4391. ⟨10.1093/mnras/stab3128⟩
Monthly Notices of the Royal Astronomical Society, 2022, 509, pp.4372-4391. ⟨10.1093/mnras/stab3128⟩
We use a sample of $z=0$ galaxies visually classified as slow rotators (SRs) in the EAGLE hydrodynamical simulations to explore the effect of galaxy mergers on their formation, characterise their intrinsic galaxy properties, and study the connection
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f01507491c68116b552f713b13e735cc
https://doi.org/10.1093/mnras/stab3128
https://doi.org/10.1093/mnras/stab3128
Autor:
K. E. Harborne, Luca Cortese, J. van de Sande, Chris Power, Aaron S. G. Robotham, Scott M. Croom, Claudia del P. Lagos
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 497:2018-2038
Observers experience a series of limitations when measuring galaxy kinematics, such as variable seeing conditions and aperture size. These effects can be reduced using empirical corrections, but these equations are usually applicable within a restric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2cf38f96a49c47aecc5a9696540a081b
https://doi.org/10.1093/mnras/staa1847
https://doi.org/10.1093/mnras/staa1847
Autor:
L Cortese, A Fraser-McKelvie, J Woo, B Catinella, K E Harborne, J van de Sande, J Bland-Hawthorn, S Brough, J J Bryant, S Croom, S Sweet
The stellar surface density within the inner 1 kpc ($\Sigma_{1}$) has become a popular tool for understanding the growth of galaxies and its connection with the quenching of star formation. The emerging picture suggests that building a central dense
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6149e2c92bb5e8a35a812ab3f3837234
Autor:
K. E. Harborne, Joss Bland-Hawthorn, Sam P. Vaughan, Luca Cortese, Angel R. Lopez-Sanchez, Anne M. Medling, Richard M. McDermid, Matt S. Owers, Julia J. Bryant, Samuel N. Richards, Sarah M. Sweet, Francesco D'Eugenio, Claudia del P. Lagos, Scott M. Croom, Sarah Brough, Caroline Foster, Jesse van de Sande, Barbara Catinella, Nicholas Scott, Brent Groves
The kinematic morphology-density relation of galaxies is normally attributed to a changing distribution of galaxy stellar masses with the local environment. However, earlier studies were largely focused on slow rotators; the dynamical properties of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::218f4eced03abb34d1b53bcb27621f29
http://arxiv.org/abs/2109.06189
http://arxiv.org/abs/2109.06189
Autor:
Anne M. Medling, Nicholas Scott, Dan S. Taranu, Brent Groves, K. E. Harborne, A. Khalid, Sam P. Vaughan, Scott M. Croom, Michael Goodwin, Joss Bland-Hawthorn, Matt S. Owers, Samuel N. Richards, Luca Cortese, Claudia del P. Lagos, Caroline Foster, Jon Lawrence, J. van de Sande, Julia J. Bryant, Sarah Brough
We use comparisons between the SAMI Galaxy Survey and equilibrium galaxy models to infer the importance of disc fading in the transition of spirals into lenticular (S0) galaxies. The local S0 population has both higher photometric concentration and l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cefe134670da423ea2979fcb57fa2b42
Autor:
Francesco D'Eugenio, Claudia del P. Lagos, C. Derkenne, J. T. Mendel, David Fisher, Chiaki Kobayashi, R. Bassett, Aaron S. G. Robotham, A. Poci, J. van de Sande, A. Khalid, Sarah M. Sweet, Scott M. Croom, A. J. Battisti, Sabine Bellstedt, E. Gjergo, Anshu Gupta, K. E. Harborne, Luke J. M. Davies, Sam P. Vaughan, Emily Wisnioski, Philip Taylor, Edward N. Taylor, L. Zanisi, Kim-Vy Tran, Sukyoung K. Yi, P. Sharda, Jonathan Bland-Hawthorn, Yingjie Peng, Tania M. Barone, James W. Trayford, Felix Schulze, Richard M. McDermid, Simon P. Driver, Sree Oh, Matthew Colless, Anna Ferré-Mateu, F. Collacchioni, Tiantian Yuan, Caroline Foster, Donghyeon J. Khim, E. J. Johnston, Rhea-Silvia Remus
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical drivers of galaxy transformation at a lookback time of 3-4 Gyr, during wh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20706abe5bcef82659fa0b0da76ce633
http://arxiv.org/abs/2011.13567
http://arxiv.org/abs/2011.13567
We present SimSpin, a new, public, software framework for generating integral field spectroscopy (IFS) data cubes from N-body/hydrodynamical simulations of galaxies, which can be compared directly with observational datasets. SimSpin provides a consi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cafe0fc70b0c0b9e588f5e028ae76c7c
http://arxiv.org/abs/2003.07641
http://arxiv.org/abs/2003.07641
Autor:
Christian Wolf, Alfonso Aragón-Salamanca, A. Böhm, Bruno Rodríguez del Pino, Steven P. Bamford, K. E. Harborne, Meghan E. Gray, Ana L. Chies-Santos, Tim Weinzirl
We study the effect of inclination on the apparent brightness of star-forming galaxies in spectral passbands that are commonly used as star-formation indicators. As diagnostics we use mass-to-light ratios in three passbands: the UV continuum at 280 n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f172fb9a2780a5feacee90054a1180b