Zobrazeno 1 - 10
of 12 561
pro vyhledávání: '"Andreani, A."'
Autor:
Booth, Mark, Klaassen, Pamela, Cicone, Claudia, Mroczkowski, Tony, Cordiner, Martin A., Di Mascolo, Luca, Johnstone, Doug, van Kampen, Eelco, Lee, Minju M., Liu, Daizhong, Orlowski-Scherer, John, Saintonge, Amélie, Smith, Matthew W. L., Thelen, Alexander, Wedemeyer, Sven, Akiyama, Kazunori, Andreon, Stefano, Arzoumanian, Doris, Bakx, Tom J. L. C., Bot, Caroline, Bower, Geoffrey, Brajša, Roman, Chen, Chian-Chou, da Cunha, Elisabete, Eden, David, Ettori, Stefano, Gaches, Brandt, Hatziminaoglou, Evanthia, Luppe, Patricia, Magnelli, Benjamin, Marshall, Jonathan P., Montenegro-Montes, Francisco Miguel, Niemack, Michael, Nixon, Conor, de Pater, Imke, Perrott, Yvette, Raimundo, Sandra I., Redaelli, Elena, Richards, Anita, Rybak, Matus, Šarčević, Nikolina, Semenov, Dmitry, Spezzano, Silvia, Srinivasan, Sundar, Stanke, Thomas, Andreani, Paola, Beltrán, Maria T., Butler, Bryan J., Cantalupo, Sebastiano, Dagostino, Miguel Chavez, Duarte-Cabral, Ana, Emonts, Bjorn, Fletcher, Leigh, Gary, Dale E., Gunar, Stanislav, Hacar, Alvaro, Hagedorn, Bendix, Kaminski, Tomek, Kirton, Fiona, de Kleer, Katherine, Kontar, Eduard, Kuan, Yi-Jehng, Lightfoot, John, Lopez-Rodriguez, Enrique, Lundgren, Andreas, Milam, Stefanie N., Mohan, Atul, Moreno, Raphael, Motorina, Galina G., Moullet, Arielle, Pattle, Kate, Pellizzoni, Alberto, Peretto, Nicolas, Ramasawmy, Joanna, Ricci, Claudio, Rigby, Andrew J., Sánchez-Monge, Álvaro, Saberi, Maryam, Shimojo, Masumi, Simionescu, Aurora, Thompson, Mark, Traficante, Alessio, Vignali, Cristian, White, Stephen M.
Submillimeter and millimeter wavelengths provide a unique view of the Universe, from the gas and dust that fills and surrounds galaxies to the chromosphere of our own Sun. Current single-dish facilities have presented a tantalising view of the bright
Externí odkaz:
http://arxiv.org/abs/2407.01413
Autor:
Ghodsi, L., Zhou, J., Andreani, P., De Breuck, C., Man, A. W. S., Miyamoto, Y., Bisbas, T. G., Lundgren, A., Zhang, Z. -Y.
The evolution of galaxies is largely affected by exchanging material with their close environment, the circumgalactic medium (CGM). In this work, we investigate the CGM and the interstellar medium (ISM) of the bright central galaxy (BCG) of the galax
Externí odkaz:
http://arxiv.org/abs/2406.09552
Autor:
Liu, Daizhong, Saintonge, Amelie, Bot, Caroline, Kemper, Francisca, Lopez-Rodriguez, Enrique, Smith, Matthew W. L., Stanke, Thomas, Andreani, Paola, Boselli, Alessandro, Cicone, Claudia, Davis, Timothy A., Hagedorn, Bendix, Lasrado, Akhil, Mao, Ann, Viti, Serena, Booth, Mark, Klaassen, Pamela, Mroczkowski, Tony, Bigiel, Frank, Chevance, Melanie, Cordiner, Martin A., Di Mascolo, Luca, Johnstone, Doug, Lee, Minju M., Maccarone, Thomas, Thelen, Alexander E., van Kampen, Eelco, Wedemeyer, Sven
Understanding the physical processes that regulate star formation and galaxy evolution are major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to inspect interstellar medium (ISM), star formation (SF), radiative
Externí odkaz:
http://arxiv.org/abs/2403.01202
Autor:
Lee, Minju M., Schimek, Alice, Cicone, Claudia, Andreani, Paola, Popping, Gergö, Sommovigo, Laura, Appleton, Philip N., Bischetti, Manuela, Cantalupo, Sebastiano, Chen, Chian-Chou, Dannerbauer, Helmut, De Breuck, Carlos, Di Mascolo, Luca, Emonts, Bjorn H. C., Hatziminaoglou, Evanthia, Pensabene, Antonio, Rizzo, Francesca, Rybak, Matus, Shen, Sijing, Lundgren, Andreas, Booth, Mark, Klaassen, Pamela, Mroczkowski, Tony, Cordiner, Martin A., Johnstone, Doug, van Kampen, Eelco, Liu, Daizhong, Maccarone, Thomas, Saintonge, Amélie, Smith, Matthew, Thelen, Alexander E., Wedemeyer, Sven
Our knowledge of galaxy formation and evolution has incredibly progressed through multi-wavelength observational constraints of the interstellar medium (ISM) of galaxies at all cosmic epochs. However, little is known about the physical properties of
Externí odkaz:
http://arxiv.org/abs/2403.00924
Autor:
Di Mascolo, Luca, Perrott, Yvette, Mroczkowski, Tony, Andreon, Stefano, Ettori, Stefano, Simionescu, Aurora, Raghunathan, Srinivasan, van Marrewijk, Joshiwa, Cicone, Claudia, Lee, Minju, Nelson, Dylan, Sommovigo, Laura, Booth, Mark, Klaassen, Pamela, Andreani, Paola, Cordiner, Martin A., Johnstone, Doug, van Kampen, Eelco, Liu, Daizhong, Maccarone, Thomas J., Morris, Thomas W., Saintonge, Amélie, Smith, Matthew, Thelen, Alexander E., Wedemeyer, Sven
An omnipresent feature of the multi-phase ``cosmic web'' is that warm/hot (>$10^5$ K) ionized gas pervades it. This gas constitutes a relevant contribution to the overall universal matter budget across multiple scales, from the several tens of Mpc-sc
Externí odkaz:
http://arxiv.org/abs/2403.00909
Autor:
Arroyave, I. Montoya, Cicone, C., Andreani, P., Weiss, A., De Breuck, C., Lundgren, A., Severgnini, P., Hagedorn, B., Rubinur, K., Baumschlager, B., Makroleivaditi, E.
Publikováno v:
A&A 686, A47 (2024)
Local ULIRGs host ubiquitous molecular outflows, including the most massive and powerful ever detected. These sources have also exceptionally excited global, galaxy-integrated CO ladders. A connection between outflows and molecular gas excitation has
Externí odkaz:
http://arxiv.org/abs/2402.17851
Autor:
Barhoumi-Andréani, Yacine
We analyse in a systematic way the occurrences of a remarkable structure in the theory of integrable probability that we call a ``max-independence structure'', when random variables are constructed as a maximum of a sequence of independent random var
Externí odkaz:
http://arxiv.org/abs/2401.08033
Autor:
Aranda, Román Fernández, Santos, Tanio Díaz, Hatziminaoglou, Evanthia, Assef, Roberto J., Aravena, Manuel, Eisenhardt, Peter R. M., Ferkinhoff, Carl, Pensabene, Antonio, Nikola, Thomas, Andreani, Paola, Vishwas, Amit, Stacey, Gordon J., Decarli, Roberto, Blain, Andrew W., Brisbin, Drew, Charmandaris, Vassilis, Jun, Hyunsung D., Li, Guodong, Liao, Mai, Martin, Lee R., Stern, Daniel, Tsai, Chao-Wei, Wu, Jingwen, Zewdie, Dejene
WISE J224607.6-052634.9 (W2246-0526) is a hot dust-obscured galaxy at $z$ = 4.601, and the most luminous obscured quasar known to date. W2246-0526 harbors a heavily obscured supermassive black hole that is most likely accreting above the Eddington li
Externí odkaz:
http://arxiv.org/abs/2401.01871
Autor:
Kolwa, S., De Breuck, C., Vernet, J., Wylezalek, D., Wang, W., Popping, G., Man, A. W. S., Harrison, C. M., Andreani, P.
We present Atacama Large Millimeter/sub-millimeter Array (ALMA) neutral carbon, [C I](1-0), line observations that probe molecular hydrogen gas (H$_2$) within seven radio galaxies at $z = 2.9 - 4.5$ surrounded by extended ($\gtrsim100$ kpc) Ly-$\alph
Externí odkaz:
http://arxiv.org/abs/2309.00459
Autor:
Yang, Chentao, Omont, Alain, Martín, Sergio, Bisbas, Thomas G., Cox, Pierre, Beelen, Alexandre, González-Alfonso, Eduardo, Gavazzi, Raphaël, Aalto, Susanne, Andreani, Paola, Ceccarelli, Cecilia, Gao, Yu, Gorski, Mark, Guélin, Michel, Fu, Hai, Ivison, R. J., Knudsen, Kirsten K., Lehnert, Matthew, Messias, Hugo, Muller, Sebastien, Neri, Roberto, Riechers, Dominik, van der Werf, Paul, Zhang, Zhi-Yu
Publikováno v:
A&A 680, A95 (2023)
Understanding the nature of high-$z$ dusty galaxies requires a comprehensive view of their ISM and molecular complexity. However, the molecular ISM at high-$z$ is commonly studied using only a few species beyond CO, limiting our understanding. In thi
Externí odkaz:
http://arxiv.org/abs/2308.07368