Zobrazeno 1 - 10
of 201
pro vyhledávání: '"CAROLLO, C. MARCELLA"'
Autor:
Brok, Mark den, Carollo, C. Marcella, Erroz-Ferrer, Santiago, Fagioli, Martina, Brinchmann, Jarle, Emsellem, Eric, Krajnović, Davor, Marino, Raffaella A., Onodera, Masato, Tacchella, Sandro, Weilbacher, Peter M., Woo, Joanna
We have obtained data for 41 star forming galaxies in the MUSE Atlas of Disks (MAD) survey with VLT/MUSE. These data allow us, at high resolution of a few 100 pc, to extract ionized gas kinematics ($V, \sigma$) of the centers of nearby star forming g
Externí odkaz:
http://arxiv.org/abs/1911.06070
Autor:
Erroz-Ferrer, Santiago, Carollo, C. Marcella, Brok, Mark den, Onodera, Masato, Brinchmann, Jarle, Marino, Raffaella A., Monreal-Ibero, Ana, Schaye, Joop, Woo, Joanna, Cibinel, Anna, Debattista, Victor P., Inami, Hanae, Maseda, Michael, Richard, Johan, Tacchella, Sandro, Wisotzki, Lutz
We study the physical properties of the ionized gas in local disks using the sample of 38 nearby $\sim10^{8.5-11.2}$M$_\odot$ Star-Forming Main Sequence (SFMS) galaxies observed so far as part of the MUSE Atlas of Disks (MAD). Specifically, we use al
Externí odkaz:
http://arxiv.org/abs/1901.04493
Kiloparsec Scale Properties of Star-Formation Driven Outflows at z~2.3 in the SINS/zC-SINF AO Survey
Autor:
Davies, Rebecca L., Schreiber, Natascha M. Förster, Übler, Hannah, Genzel, Reinhard, Lutz, Dieter, Renzini, Alvio, Tacchella, Sandro, Tacconi, Linda J., Belli, Sirio, Burkert, Andreas, Carollo, C. Marcella, Davies, Richard I., Herrera-Camus, Rodrigo, Lilly, Simon J., Mancini, Chiara, Naab, Thorsten, Nelson, Erica J., Price, Sedona H., Shimizu, Thomas Taro, Sternberg, Amiel, Wisnioski, Emily, Wuyts, Stijn
We investigate the relationship between star formation activity and outflow properties on kiloparsec scales in a sample of 28 star forming galaxies at $z\sim$ 2-2.6, using adaptive optics assisted integral field observations from SINFONI on the VLT.
Externí odkaz:
http://arxiv.org/abs/1808.10700
Autor:
Giesers, Benjamin, Dreizler, Stefan, Husser, Tim-Oliver, Kamann, Sebastian, Escude, Guillem Anglada, Brinchmann, Jarle, Carollo, C. Marcella, Roth, Martin M., Weilbacher, Peter M., Wisotzki, Lutz
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters, Volume 475, Issue 1, 21 March 2018, Pages L15-L19
As part of our massive spectroscopic survey of 25 Galactic globular clusters with MUSE, we performed multiple epoch observations of NGC 3201 with the aim of constraining the binary fraction. In this cluster, we found one curious star at the main-sequ
Externí odkaz:
http://arxiv.org/abs/1801.05642
Autor:
Molnar, Daniel Cs., Sargent, Mark T., Delhaize, Jacinta, Delvecchio, Ivan, Smolcic, Vernesa, Novak, Mladen, Schinnerer, Eva, Zamorani, Giovanni, Bondi, Marco, Herrera-Ruiz, Noelia, Murphy, Eric J., Vardoulaki, Eleni, Karim, Alexander, Leslie, Sarah, Magnelli, Benjamin, Carollo, C. Marcella, Middelberg, Enno
Using infrared data from the Herschel Space Observatory and Karl G. Jansky Very Large Array (VLA) 3 GHz observations in the COSMOS field, we investigate the redshift evolution of the infrared-radio correlation (IRRC) for star-forming galaxies (SFGs)
Externí odkaz:
http://arxiv.org/abs/1710.07655
Autor:
Marino, Raffaella Anna, Cantalupo, Sebastiano, Lilly, Simon J., Gallego, Sofia G., Straka, Lorrie A., Borisova, Elena, Bacon, Roland, Brinchmann, Jarle, Carollo, C. Marcella, Caruana, Joseph, Conseil, Simon, Contini, Thierry, Diener, Catrina, Finley, Hayley, Inami, Hanae, Leclercq, Floriane, Muzahid, Sowgat, Richard, Johan, Schaye, Joop, Wendt, Martin, Wisotzki, Lutz
Recent theoretical models suggest that the early phase of galaxy formation could involve an epoch when galaxies are gas-rich but inefficient at forming stars: a "dark galaxy" phase. Here, we report the results of our MUSE (Multi Unit Spectroscopic Ex
Externí odkaz:
http://arxiv.org/abs/1709.03522
Autor:
Tacchella, Sandro, Carollo, C. Marcella, Faber, S. M., Cibinel, Anna, Dekel, Avishai, Koo, David C., Renzini, Alvio, Woo, Joanna
We investigate the origin of the evolution of the population-averaged central stellar mass density ($\Sigma_1$) of quiescent galaxies (QGs) by probing the relation between stellar age and $\Sigma_1$ at $z\sim0$. We use the Zurich ENvironmental Study
Externí odkaz:
http://arxiv.org/abs/1707.00695
Autor:
Mosleh, Moein, Tacchella, Sandro, Renzini, Alvio, Carollo, C. Marcella, Molaeinezhad, Alireza, Onodera, Masato, Khosroshahi, Habib G., Lilly, Simon
We study the history from $z\sim2$ to $z\sim0$ of the stellar mass assembly of quiescent and star-forming galaxies in a spatially resolved fashion. For this purpose we use multi-wavelength imaging data from the Hubble Space Telescope (HST) over the G
Externí odkaz:
http://arxiv.org/abs/1702.02392
Autor:
Fagioli, Martina, Carollo, C. Marcella, Renzini, Alvio, Lilly, Simon J., Onodera, Masato, Tacchella, Sandro
We investigate the origin of the evolution of the population-averaged size of quenched galaxies (QGs) through a spectroscopic analysis of their stellar ages. The two most favoured scenarios for this evolution are either the size growth of individual
Externí odkaz:
http://arxiv.org/abs/1607.03493
Autor:
Borisova, Elena, Cantalupo, Sebastiano, Lilly, Simon J., Marino, Raffaella A., Gallego, Sofia G., Bacon, Roland, Blaizot, Jeremy, Bouché, Nicolas, Brinchmann, Jarle, Carollo, C. Marcella, Caruana, Joseph, Finley, Hayley, Herenz, Edmund C., Richard, Johan, Schaye, Joop, Straka, Lorrie A., Turner, Monica L., Urrutia, Tanya, Verhamme, Anne, Wisotzki, Lutz
Direct Ly $\alpha$ imaging of intergalactic gas at $z\sim2$ has recently revealed giant cosmological structures around quasars, e.g. the Slug Nebula (Cantalupo et al. 2014). Despite their high luminosity, the detection rate of such systems in narrow-
Externí odkaz:
http://arxiv.org/abs/1605.01422