Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Pierre-Yves Lablanche"'
Autor:
Michelle Lochner, Shankar Agarwal, José Fonseca, Bruce A. Bassett, Pierre-Yves Lablanche, Ethan Roberts
Supernova cosmology without spectra will be an important component of future surveys such as LSST. This lack of supernova spectra results in uncertainty in the redshifts which, if ignored, leads to significantly biased estimates of cosmological param
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8faef6126d30bd9097cb6fcdd5d8cfc
Autor:
M. Bois, Pierre-Alain Duc, Davor Krajnović, Katherine Alatalo, Pierre Yves Lablanche, Richard M. McDermid, Michele Cappellari, Sadegh Khochfar, Eric Emsellem, Lisa M. Young, Tom Oosterloo, Alison F. Crocker, Paolo Serra, Raffaella Morganti, P. T. de Zeeuw, Nicholas Scott, Anne-Marie Weijmans, Roger L. Davies, Timothy A. Davis, Thorsten Naab, Martin Bureau, Marc Sarzi, Harald Kuntschner, Leo Blitz, Frédéric Bournaud
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2013, 432 (3), pp.1845-1861. ⟨10.1093/mnras/stt062⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 432 (3), pp.1845-1861. ⟨10.1093/mnras/stt062⟩
Monthly Notices of the Royal Astronomical Society, 432(3), 1845-1861. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 2013, 432 (3), pp.1845-1861. ⟨10.1093/mnras/stt062⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2013, 432 (3), pp.1845-1861. ⟨10.1093/mnras/stt062⟩
Monthly Notices of the Royal Astronomical Society, 432(3), 1845-1861. Oxford University Press
For early-type galaxies, the ability to sustain a corona of hot, X-ray emitting gas could have played a key role in quenching their star-formation history. Yet, it is still unclear what drives the precise amount of hot gas around these galaxies. By c
Autor:
Thorsten Naab, Nicholas Scott, Harald Kuntschner, Martin Bureau, Marc Sarzi, M. Bois, Davor Krajnović, Leo Blitz, Katherine Alatalo, Roger L. Davies, Paolo Serra, Sadegh Khochfar, Jesús Falcón-Barroso, Pierre Yves Lablanche, P. T. de Zeeuw, Anne-Marie Weijmans, Frédéric Bournaud, R. C. E. van den Bosch, E. Emsellem, Michele Cappellari, Timothy A. Davis, Richard M. McDermid, Raffaella Morganti, G. van de Ven, Lisa M. Young
Publikováno v:
Highlights of Astronomy, 15
We study the origin of the scaling relations of early-type galaxies (ETGs) by constructing detailed models of the stellar dynamics for the K-band selected, volume-limited ATLAS3D sample of 263 nearby ETGs, spanning a large range of masses and stellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::742187edb6c667f1c5eeae9cab4c151e
https://ora.ox.ac.uk/objects/uuid:17ec5ed2-c792-4706-a535-3757c6955a0d
https://ora.ox.ac.uk/objects/uuid:17ec5ed2-c792-4706-a535-3757c6955a0d
Autor:
Raffaella Morganti, Katherine Alatalo, E. Bayet, Kristina Nyland, Roger L. Davies, Thorsten Naab, Paolo Serra, Leo Blitz, Eric Emsellem, Sadegh Khochfar, Martin Bureau, Marc Sarzi, P. T. de Zeeuw, Tom Oosterloo, Alison F. Crocker, Michele Cappellari, Pierre-Alain Duc, Anne-Marie Weijmans, Lisa M. Young, Davor Krajnović, Pierre Yves Lablanche, Maxime Bois, Richard M. McDermid, Frédéric Bournaud, Harald Kuntschner, Nicholas Scott, Timothy A. Davis
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 426:1574-1590
We use the SAURON and GMOS integral field spectrographs to observe the active galactic nucleus (AGN) powered outflow in NGC 1266. This unusual galaxy is relatively nearby (D=30 Mpc), allowing us to investigate the process of AGN feedback in action. W
Autor:
Pierre-Alain Duc, Thorsten Naab, E. Bayet, Richard M. McDermid, Anne-Marie Weijmans, Paolo Serra, Maxime Bois, Frédéric Bournaud, Michele Cappellari, Timothy A. Davis, Martin Bureau, Marc Sarzi, P. T. de Zeeuw, Lisa M. Young, Tom Oosterloo, Harald Kuntschner, Davor Krajnović, Nicholas Scott, Roger L. Davies, Pierre Yves Lablanche, Leo Blitz, Sadegh Khochfar, Eric Emsellem, Alison F. Crocker, Raffaella Morganti, Katherine Alatalo, Melanie Krips
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 421:1298-1314
Surveying eighteen 12CO-bright galaxies from the ATLAS3D early-type galaxy sample with the Institut de Radio Astronomie Millim\'etrique (IRAM) 30m telescope, we detect 13CO(1-0) and 13CO(2-1) in all eighteen galaxies, HCN(1-0) in 12/18 and HCO+(1-0)
Autor:
Eric Emsellem, Katherine Alatalo, Davor Krajnović, Roger L. Davies, Michele Cappellari, Pierre Yves Lablanche, Thorsten Naab, Sadegh Khochfar, Timothy A. Davis, Leo Blitz, Martin Bureau, Marc Sarzi, Nicholas Scott, Richard M. McDermid, Anne-Marie Weijmans, Raffaella Morganti, Frédéric Bournaud, Paolo Serra, Lisa M. Young, Maxime Bois, Harald Kuntschner, P. T. de Zeeuw, Tom Oosterloo
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 416:1680-1696
We look at the morphology of fast and slow rotator early-type galaxies. Edge-on fast rotators are lenticular galaxies. They appear like spiral galaxies with the gas and dust removed, and in some cases are flat ellipticals with disky isophotes. Fast r
Autor:
Sadegh Khochfar, Tom Oosterloo, Timothy A. Davis, Davor Krajnović, Eric Emsellem, Pierre Yves Lablanche, Harald Kuntschner, Katherine Alatalo, Frédéric Bournaud, Nicholas Scott, Paolo Serra, Lisa M. Young, Roger L. Davies, Thorsten Naab, P. T. de Zeeuw, Raffaella Morganti, Maxime Bois, Martin Bureau, Marc Sarzi, Leo Blitz, Michele Cappellari, Richard M. McDermid, Anne-Marie Weijmans, Pierre-Alain Duc
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 416:1654-1679
We study the formation of early-type galaxies through mergers with a sample of 70 high-resolution (softening length < 60 pc and 12*10^6 particles) numerical simulations of binary mergers of disc galaxies and 16 simulations of ETG remergers. These sim
Autor:
Paolo Serra, Raffaella Morganti, Maxime Bois, Nicholas Scott, Frédéric Bournaud, Sadegh Khochfar, Davor Krajnović, Pierre Yves Lablanche, Thorsten Naab, Leo Blitz, Harald Kuntschner, Richard M. McDermid, Lisa M. Young, Eric Emsellem, Michele Cappellari, Timothy A. Davis, Martin Bureau, Marc Sarzi, Katherine Alatalo, Roger L. Davies, Anne-Marie Weijmans, P. T. de Zeeuw, Tom Oosterloo
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 414:2923-2949
[Abridged] We use the ATLAS3D sample of 260 early-type galaxies (ETGs) to study the apparent kinematic misalignment angle, Psi, defined as the angle between the photometric and kinematic major axis. We find that 71% of nearby ETGs are strictly aligne
Autor:
Raffaella Morganti, Harald Kuntschner, Katherine Alatalo, Timothy A. Davis, Paolo Serra, Martin Bureau, Marc Sarzi, Michele Cappellari, Lisa M. Young, Leo Blitz, Roger L. Davies, Nicholas Scott, Sadegh Khochfar, Tom Oosterloo, Eric Emsellem, Richard M. McDermid, P. Tim de Zeeuw, Anne-Marie Weijmans, Thorsten Naab, Frédéric Bournaud, Pierre Yves Lablanche, Davor Krajnović, Maxime Bois
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 414:968-984
We demonstrate here using both single-dish and interferometric observations that CO molecules are an excellent kinematic tracer, even in high-mass galaxies, allowing us to investigate for the first time the CO Tully-Fisher relation of early-type gala
Autor:
Pierre Yves Lablanche, Raffaella Morganti, P. T. de Zeeuw, Anne-Marie Weijmans, Eric Emsellem, Sadegh Khochfar, Paolo Serra, Harald Kuntschner, Nicholas Scott, Katherine Alatalo, Richard M. McDermid, Davor Krajnović, Tom Oosterloo, Roger L. Davies, Francoise Combes, Michele Cappellari, Thorsten Naab, Martin Bureau, Marc Sarzi, Frédéric Bournaud, Leo Blitz, Maxime Bois, Lisa M. Young, Timothy A. Davis
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 414:940-967
We have carried out a survey for 12CO J=1-0 and J=2-1 emission in the 260 early-type galaxies of the volume-limited Atlas3D sample, with the goal of connecting their star formation and assembly histories to their cold gas content. This is the largest