| dc.contributor.author | Falcon-Barroso, J. | |
| dc.contributor.author | Bacon, R. | |
| dc.contributor.author | Cappellari, M. | |
| dc.contributor.author | Davies, R.L. | |
| dc.contributor.author | de Zeeuw, P.T. | |
| dc.contributor.author | Emsellem, E. | |
| dc.contributor.author | Krajnovic, D. | |
| dc.contributor.author | Kuntschner, H. | |
| dc.contributor.author | McDermid, R.M. | |
| dc.contributor.author | Peletier, R.F. | |
| dc.contributor.author | Sarzi, M. | |
| dc.contributor.author | van de Ven, G. | |
| dc.date.accessioned | 2008-06-27T14:18:47Z | |
| dc.date.available | 2008-06-27T14:18:47Z | |
| dc.date.issued | 2008 | |
| dc.identifier.citation | Falcon-Barroso , J , Bacon , R , Cappellari , M , Davies , R L , de Zeeuw , P T , Emsellem , E , Krajnovic , D , Kuntschner , H , McDermid , R M , Peletier , R F , Sarzi , M & van de Ven , G 2008 , Towards a New Classification of Early-type Galaxies: An Integral-field View . in In: Pathways Through an Eclectic Universe - ASP Conf Series 390 . Astronomical Society of the Pacific , pp. 227-231 . | |
| dc.identifier.isbn | 978-1-58381-651-6 | |
| dc.identifier.isbn | 978-1-58381-650-9 | |
| dc.identifier.other | PURE: 138392 | |
| dc.identifier.other | PURE UUID: a7caf54c-0c1f-48df-9319-db59f94b34bf | |
| dc.identifier.other | dspace: 2299/2162 | |
| dc.identifier.uri | http://hdl.handle.net/2299/2162 | |
| dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASP | |
| dc.description.abstract | In this proceedings paper we make use of the two-dimensional stel- lar kinematics of a representative sample of E and S0 galaxies obtained with the SAURON integral-field spectrograph to reveal that early-type galaxies appear in two broad flavors, depending on whether they exhibit clear large-scale rotation or not. We measure the level of rotation via a new parameter (λR) and use it as a basis for a new kinematic classification that separates early-type galaxies into slow and fast rotators. With the aid of broad-band imaging we will reinforce this finding by comparing our kinematic results to the photometric properties of these two classes. | en |
| dc.language.iso | eng | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.ispartof | In: Pathways Through an Eclectic Universe - ASP Conf Series 390 | |
| dc.title | Towards a New Classification of Early-type Galaxies: An Integral-field View | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
