Zobrazeno 1 - 10
of 1 654
pro vyhledávání: '"Romano, Michael A."'
Autor:
Killi, Meghana, Ginolfi, Michele, Popping, Gergö, Watson, Darach, Zamorani, Giovanni, Lemaux, Brian C., Fujimoto, Seiji, Faisst, Andreas, Bethermin, Matthieu, Romano, Michael, Fudamoto, Yoshinobu, Bardelli, Sandro, Boquien, Médéric, Carniani, Stefano, Dessauges-Zavadsky, Miroslava, Gruppioni, Carlotta, Hathi, Nimish, Ibar, Eduardo, Jones, Gareth C., Koekemoer, Anton M., Langan, Ivanna, Méndez-Hernández, Hugo, Sugahara, Yuma, Vallini, Livia, Vergani, Daniela
Galaxy morphology is shaped by stellar activity, feedback, gas and dust properties, and interactions with surroundings, and can therefore provide insight into these processes. In this paper, we study the spatial offsets between stellar and interstell
Externí odkaz:
http://arxiv.org/abs/2402.07982
Autor:
Nanni, Ambra, Cristallo, Sergio, Donevski, Darko, Michałowski, Michał J., Romano, Michael, Sawant, Prasad
Aims. We investigate the role of photo-evaporation of dust exposed to the radiation field from hot young stars and planetary nebulae (PNe) as a possible destruction mechanism of dust grains in the interstellar medium (ISM). Methods. We estimate photo
Externí odkaz:
http://arxiv.org/abs/2312.15998
Autor:
Romano, Michael, Nanni, Ambra, Donevski, Darko, Ginolfi, Michele, Jones, Gareth C., Shivaei, Irene, Junais, Salak, Dragan, Sawant, Prasad
Publikováno v:
A&A 677, A44 (2023)
We characterize the physical properties of star-formation driven outflows in a sample of 29 local dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to search for atomic outflow signatures in the wings of in
Externí odkaz:
http://arxiv.org/abs/2306.10433
Autor:
Donevski, Darko, Damjanov, Ivana, Nanni, Ambra, Man, Allison, Giulietti, Marika, Romano, Michael, Lapi, Andrea, Narayanan, Desika, Davé, Romeel, Shivaei, Irene, Sohn, Jubee, Junais, Pantoni, Lara, Li, Qi
Publikováno v:
A&A 678, A35 (2023)
Quantifying changes in galaxies' interstellar medium (ISM) abundance after quenching star formation is an important aspect of galaxy evolution, but it is poorly constrained beyond the local universe. We characterise the dust-related properties in 548
Externí odkaz:
http://arxiv.org/abs/2304.05842
Autor:
Shen, Lu, Lemaux, Brian C., Lubin, Lori M., Liu, Guilin, Béthermin, Matthieu, Boquien, Médéric, Cucciati, Olga, Fèvre, Olivier Le, Talia, Margherita, Vergani, Daniela, Zamorani, Gianni, Faisst, Andreas L., Ginolfi, Michele, Gruppioni, Carlotta, Jones, Gareth C., Bardelli, Sandro, Hathi, Nimish, Koekemoer, Anton M., Romano, Michael, Schaerer, Daniel, Zucca, Elena, Fang, Wenjuan, Forrest, Ben, Gal, Roy, Hung, Denise, Shah, Ekta A., Staab, Priti, Vanderhoof, Brittany, Ibar, Eduardo
We present the radio properties of 66 spectroscopically-confirmed normal star-forming galaxies (SFGs) at $4.4
Externí odkaz:
http://arxiv.org/abs/2207.07137
Autor:
Boquien, Mederic, Buat, Veronique, Burgarella, Denis, Bardelli, Sandro, Bethermin, Matthieu, Faisst, Andreas, Ginolfi, Michele, Hathi, Nimish, Jones, Gareth, Koekemoer, Anton, Lemaux, Brian, Narayanan, Desika, Romano, Michael, Schaerer, Daniel, Vergani, Daniela, Zamorani, Giovanni, Zucca, Elena
Publikováno v:
A&A 663, A50 (2022)
There is now ample evidence that dust is already present in abundance at high z. However, given the faintness of distant galaxies in the optical and the NIR, datasets are still limited and how the dust affects the emerging radiation of galaxies at ve
Externí odkaz:
http://arxiv.org/abs/2202.11723
Autor:
Romano, Michael, Morselli, L., Cassata, P., Ginolfi, M., Schaerer, D., Béthermin, M., Capak, P., Faisst, A., Fèvre, O. Le, Silverman, J. D., Yan, L., Bardelli, S., Boquien, M., Dessauges-Zavadsky, M., Fujimoto, S., Hathi, N. P., Jones, G. C., Koekemoer, A. M., Lemaux, B. C., Méndez-Hernández, H., Narayanan, D., Talia, M., Vergani, D., Zamorani, G., Zucca, E.
Publikováno v:
A&A 660, A14 (2022)
The [CII] 158$~\mu$m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brightest cooling lines in the rest-frame far-infrared regime of star-fo
Externí odkaz:
http://arxiv.org/abs/2202.02334
Autor:
Loiacono, Federica, Decarli, Roberto, Gruppioni, Carlotta, Talia, Margherita, Cimatti, Andrea, Zamorani, Gianni, Pozzi, Francesca, Yan, Lin, Lemaux, Brian C., Riechers, Dominik A., Fèvre, Olivier Le, Béthermin, Matthieu, Capak, Peter, Cassata, Paolo, Faisst, Andreas, Schaerer, Daniel, Silverman, John D., Bardelli, Sandro, Boquien, Médéric, Burkutean, Sandra, Dessauges-Zavadsky, Miroslava, Fudamoto, Yoshinobu, Fujimoto, Seiji, Ginolfi, Michele, Hathi, Nimish P., Jones, Gareth C., Khusanova, Yana, Koekemoer, Anton M., Lagache, Guilaine, Massardi, Marcella, Oesch, Pascal, Romano, Michael, Vallini, Livia, Vergani, Daniela, Zucca, Elena
Publikováno v:
A&A 646, A76 (2021)
We present the first [CII] 158 $\mu$m luminosity function (LF) at $z\sim 5$ from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). A search performed over the 118 ALPINE pointings reveale
Externí odkaz:
http://arxiv.org/abs/2006.04837
Autor:
Morselli, Laura, Rodighiero, Giulia, Enia, Andrea, Corbelli, Edvige, Casasola, Viviana, Rodriguez-Muñoz, Lucia, Renzini, Alvio, Tacchella, Sandro, Baronchelli, Ivano, Bianchi, Simone, Cassata, Paolo, Franceschini, Alberto, Mancini, Chiara, Negrello, Mattia, Popesso, Paola, Romano, Michael
In the second work of this series, we analyse the connection between the availability of gas and the position of a region with respect to the spatially resolved main sequence (MS) relation. Following the procedure presented in Paper I we obtain 500pc
Externí odkaz:
http://arxiv.org/abs/2003.02861
Autor:
Cassata, Paolo, Liu, Daizhong, Groves, Brent, Schinnerer, Eva, Ibar, Eduardo, Sargent, Mark, Karim, Alexander, Talia, Margherita, Fevre, Olivier Le, Tasca, Lidia, Lemaux, Brian C., Ribeiro, Bruno, Fiore, Stefano, Romano, Michael, Mancini, Chiara, Morselli, Laura, Rodighiero, Giulia, Rodriguez-Munoz, Lucia, Enia, Andrea, Smolcic, Vernesa
We present the detection of CO(5-4) with S/N> 7 - 13 and a lower CO transition with S/N > 3 (CO(4-3) for 4 galaxies, and CO(3-2) for one) with ALMA in band 3 and 4 in five main sequence star-forming galaxies with stellar masses 3-6x10^10 M/M_sun at 3
Externí odkaz:
http://arxiv.org/abs/2002.04040