Michele Cappellari: Publications

A way to deal with the fringe-like pattern in VIMOS-IFU data

(2012)

Authors:

Carina Lagerholm, Harald Kuntschner, Michele Cappellari, Davor Krajnovic, Richard McDermid, Marina Rejkuba

A systematic variation of the stellar initial mass function in early-type galaxies

(2012)

Authors:

Michele Cappellari, Richard M McDermid, Katherine Alatalo, Leo Blitz, Maxime Bois, Frederic Bournaud, M Bureau, Alison F Crocker, Roger L Davies, Timothy A Davis, PT de Zeeuw, Pierre-Alain Duc, Eric Emsellem, Sadegh Khochfar, Davor Krajnovic, Harald Kuntschner, Pierre-Yves Lablanche, Raffaella Morganti, Thorsten Naab, Tom Oosterloo, Marc Sarzi, Nicholas Scott, Paolo Serra, Anne-Marie Weijmans, Lisa M Young

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The SAURON project – XX. The Spitzer [3.6] − [4.5] colour in early-type galaxies: colours, colour gradients and inverted scaling relations

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 419:3 (2012) 2031-2053

Authors:

Reynier F Peletier, Elif Kutdemir, Guido van der Wolk, Jesús Falcón-Barroso, Roland Bacon, Martin Bureau, Michele Cappellari, Roger L Davies, P Tim de Zeeuw, Eric Emsellem, Davor Krajnović, Harald Kuntschner, Richard M McDermid, Marc Sarzi, Nicholas Scott, Kristen L Shapiro, Remco CE van den Bosch, Glenn van de Ven

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Simulations of binary galaxy mergers and the link with Fast Rotators, Slow Rotators, and Kinematically Distinct Cores

(2012)

Authors:

Maxime Bois, Eric Emsellem, Frédéric Bournaud, Katherine Alatalo, Leo Blitz, Martin Bureau, Michele Cappellari, Roger L Davies, Timothy A Davis, PT de Zeeuw, Pierre-Alain Duc, Sadegh Khochfar, Davor Krajnović, Harald Kuntschner, Pierre-Yves Lablanche, Richard M McDermid, Raffaella Morganti, Thorsten Naab, Tom Oosterloo, Marc Sarzi, Nicholas Scott, Paolo Serra, Anne-Marie Weijmans, Lisa M Young

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Dynamical masses of early-type galaxies at z ∼ 2

Proceedings of the International Astronomical Union 8:S295 (2012) 37-44

Abstract:

The evolution of masses and sizes of passive (early-type) galaxies with redshift provides ideal constraints to galaxy formation models. These parameters can in principle be obtained for large galaxy samples from multi-band photometry alone. However the accuracy of photometric masses is limited by the non-universality of the IMF. Galaxy sizes can be biased at high redshift due to the inferior quality of the imaging data. Both problems can be avoided using galaxy dynamics, and in particular by measuring the galaxies stellar velocity dispersion. Here we provide an overview of the efforts in this direction. © 2013 International Astronomical Union.

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Michele Cappellari

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A way to deal with the fringe-like pattern in VIMOS-IFU data

Authors:

A systematic variation of the stellar initial mass function in early-type galaxies

Authors:

The SAURON project – XX. The Spitzer [3.6] − [4.5] colour in early-type galaxies: colours, colour gradients and inverted scaling relations

Authors:

Simulations of binary galaxy mergers and the link with Fast Rotators, Slow Rotators, and Kinematically Distinct Cores

Authors:

Dynamical masses of early-type galaxies at z ∼ 2

Abstract:

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Michele Cappellari

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A way to deal with the fringe-like pattern in VIMOS-IFU data

Authors:

A systematic variation of the stellar initial mass function in early-type galaxies

Authors:

The SAURON project – XX. The Spitzer [3.6] − [4.5] colour in early-type galaxies: colours, colour gradients and inverted scaling relations

Authors:

Simulations of binary galaxy mergers and the link with Fast Rotators, Slow Rotators, and Kinematically Distinct Cores

Authors:

Dynamical masses of early-type galaxies at z ∼ 2

Abstract: