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Your search keyword '"ARNABOLDI M."' showing total 11 results
Start Over Author "ARNABOLDI M." Journal proceedings of the international astronomical union
11 results on '"ARNABOLDI M."'

4. Kinematic properties of early type galaxy halos using planetary nebulae

Author

Coccato, L., primary, Gerhard, O., additional, Arnaboldi, M., additional, Das, P., additional, Douglas, N. G., additional, Kuijken, K., additional, Merrifield, M. R., additional, Napolitano, N. R., additional, Noordermeer, E., additional, Romanowsky, A. J., additional, Capaccioli, M., additional, Cortesi, A., additional, and Lorenzi, F. De, additional

Published
2009
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6. Constraining the internal dynamics of stellar systems using the NMAGIC particle code

Author

De Lorenzi, Flavio, primary, Gerhard, Ortwin, additional, Debattista, Victor P., additional, Sambhus, Niranjan, additional, Coccato, L., additional, Arnaboldi, M., additional, Capaccioli, M., additional, Douglas, N. G., additional, Freeman, K. C., additional, Kuijken, K., additional, Merrifield, M. R., additional, Napolitano, N. R., additional, Noordermeer, E., additional, and Romanowsky, A. J., additional

Published
2007
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7. Dark-Matter Content of Early-Type Galaxies with Planetary Nebulae

Author

Napolitano, N. R., primary, Romanowsky, A. J., additional, Coccato, L., additional, Capaccioli, M., additional, Douglas, N. G., additional, Noordermeer, E., additional, Merrifield, M. R., additional, Kuijken, K., additional, Arnaboldi, M., additional, Gerhard, O., additional, Freeman, K. C., additional, De Lorenzi, F., additional, and Das, P., additional

Published
2007
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10. The Vimos-VLT Deep Survey: Results from the First-Epoch Observations

Author

Paltani, S., primary, Ilbert, O., additional, Fèvre, O. Le, additional, Marinoni, C., additional, Bottini, D., additional, Garilli, B., additional, Brun, V. Le, additional, Maccagni, D., additional, Picat, J.-P., additional, Scaramella, R., additional, Scodeggio, M., additional, Tresse, L., additional, Vettolani, G., additional, Zanichelli, A., additional, Adami, C., additional, Arnaboldi, M., additional, Arnouts, S., additional, Bardelli, S., additional, Bolzonella, M., additional, Cappi, A., additional, Charlot, S., additional, Contini, T., additional, Foucaud, S., additional, Franzetti, P., additional, Gavignaud, I., additional, Guzzo, L., additional, Iovino, A., additional, McCracken, H.J., additional, Marano, B., additional, Mazure, A., additional, Meneux, B., additional, Merighi, R., additional, Pellò, R., additional, Pollo, A., additional, Pozzetti, L., additional, Radovich, M., additional, Zamorani, G., additional, Zucca, E., additional, Bondi, M., additional, Bongiorno, A., additional, Busarello, G., additional, Ciliegi, P., additional, Gregorini, L., additional, Mathez, G., additional, Mellier, Y., additional, Merluzzi, P., additional, Ripepi, V., additional, and Rizzo, D., additional

Published
2004
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11. The co-responsibility of mass and environment in the formation of lenticular galaxies.

Author

Cortesi, A., Coccato, L., Buzzo, M. L., Menéndez-Delmestre, K., Goncalves, T., Mendes de Oliveira, C., Merrifield, M., Arnaboldi, M., Bergmann, Thaisa Storchi, Forman, William, Overzier, Roderik, and Riffel, Rogério

Abstract

We present the latest data release of the Planetary Nebulae Spectrograph Survey (PNS) of ten lenticular galaxies and two spiral galaxies. With this data set we are able to recover the galaxies' kinematics out to several effective radii. We use a maximum likelihood method to decompose the disk and spheroid kinematics and we compare it with the kinematics of spiral and elliptical galaxies. We build the Tully- Fisher (TF) relation for these galaxies and we compare with data from the literature and simulations. We find that the disks of lenticular galaxies are hotter than the disks of spiral galaxies at low redshifts, but still dominated by rotation velocity. The mechanism responsible for the formation of these lenticular galaxies is neither major mergers, nor a gentle quenching driven by stripping or Active Galactic Nuclei (AGN) feedback. [ABSTRACT FROM AUTHOR]

Published
2019
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