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The SAURON project - XIII. SAURON-GALEX study of early-type galaxies: the ultraviolet colour-magnitude relations and Fundamental Planes

(2009)

Authors:

Hyunjin Jeong, Sukyoung K Yi, Martin Bureau, Roger L Davies, Jesus Falcon-Barroso, Glenn van de Ven, Reynier F Peletier, Roland Bacon, Michele Cappellari, Tim de Zeeuw, Eric Emsellem, Davor Krajnovic, Harald Kuntschner, Richard M McDermid, Marc Sarzi, Remco CE van den Bosch
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The SAURON Project - XIV. No escape from V$_{\mathrm{esc}}$: a global and local parameter in early-type galaxy evolution

(2009)

Authors:

Nicholas Scott, Michele Cappellari, Roger L Davies, R Bacon, PT de Zeeuw, Eric Emsellem, Jesus Falcon-Barroso, Davor Krajnovic, Harald Kuntschner, Richard M McDermid, Reynier F Peletier, Antonio Pipino, Marc Sarzi, Remco CE van den Bosch, Glenn van de Ven, Eveline van Scherpenzeel
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Stellar velocity profiles and line strengths out to four effective radii in the early-type galaxies NGC 3379 and NGC 821

(2009)

Authors:

A Weijmans, M Cappellari, R Bacon, PT de Zeeuw, E Emsellem, J Falcon-Barroso, H Kuntschner, RM McDermid, RCE van den Bosch, G van de Ven
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The monitor project: A search for low mass ebs in the young open cluster M50

Aip Conference Proceedings 1094 (2009) 832-835

Authors:

JL Birkby, ST Hodgkin, S Aigrain, J Irwin

Abstract:

We present preliminary results from a high-cadence photometric monitoring survey of the 130 Myr old open cluster M50. Using the semi-automated occultation detection process developed by Miller et al. [1], we uncovered eight low mass (< 1M⊙) eclipsing binary candidates in the cluster. Preliminary analysis of spectroscopic follow-up on five of these candidates confirms their binary nature. One candidate also exhibits a systemic velocity broadly consistent with the cluster radial velocity, indicating cluster membership. Confirmation of these eight candidates as true members of the M50 cluster will allow us to provide important constraints to the mass-radius relationship for objects below 1M⊙ at ages younger than lGyr, where current observations remain scarce. © 2009 American Institute of Physics.
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A Shared Tully-Fisher Relation for Spiral and S0 Galaxies

(2009)

Authors:

Michael J Williams, Martin Bureau, Michele Cappellari
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