Zobrazeno 1 - 10
of 93
pro vyhledávání: '"Tress, Robin"'
Autor:
Durán-Camacho, Eva, Duarte-Cabral, Ana, Pettitt, Alex R., Treß, Robin G., Clark, Paul C., Klessen, Ralf S., Bogue, Kamran R. J., Smith, Rowan J., Sormani, Mattia C.
To advance our understanding of the evolution of the interstellar medium (ISM) of our Galaxy, numerical models of Milky Way (MW) type galaxies are widely used. However, most models only vaguely resemble the MW (e.g. in total mass), and often use impo
Externí odkaz:
http://arxiv.org/abs/2405.09503
Autor:
Hunter, Glen H., Sormani, Mattia C., Beckmann, Jan P., Vasiliev, Eugene, Glover, Simon C. O., Klessen, Ralf S., Soler, Juan D., Brucy, Noé, Girichidis, Philipp, Göller, Junia, Ohlin, Loke, Tress, Robin, Molinari, Sergio, Gerhard, Ortwin, Benedettini, Milena, Smith, Rowan, Hennebelle, Patrick, Testi, Leonardo
Obtaining reliable distance estimates to gas clouds within the Milky Way is challenging in the absence of certain tracers. The kinematic distance approach has been used as an alternative, derived from the assumption of circular trajectories around th
Externí odkaz:
http://arxiv.org/abs/2403.18000
Autor:
Colman, Tine, Brucy, Noé, Girichidis, Philipp, Glover, Simon C. O, Benedettini, Milena, Soler, Juan D., Tress, Robin G., Traficante, Alessio, Hennebelle, Patrick, Klessen, Ralf S., Molinari, Sergio, Miville-Deschênes, Marc-Antoine
Publikováno v:
A&A 686, A155 (2024)
Molecular clouds (MC) are structures of dense gas in the interstellar medium (ISM), that extend from ten to a few hundred parsecs and form the main gas reservoir available for star formation. Hydrodynamical simulations of varying complexity are a pro
Externí odkaz:
http://arxiv.org/abs/2403.00512
Autor:
Sun, Jiayi, He, Hao, Batschkun, Kyle, Levy, Rebecca C., Emig, Kimberly, Rodriguez, M. Jimena, Hassani, Hamid, Leroy, Adam K., Schinnerer, Eva, Ostriker, Eve C., Wilson, Christine D., Bolatto, Alberto D., Mills, Elisabeth A. C., Rosolowsky, Erik, Lee, Janice C., Dale, Daniel A., Larson, Kirsten L., Thilker, David A., Ubeda, Leonardo, Whitmore, Bradley C., Williams, Thomas G., Barnes, Ashley. T., Bigiel, Frank, Chevance, Melanie, Glover, Simon C. O., Grasha, Kathryn, Groves, Brent, Henshaw, Jonathan D., Indebetouw, Remy, Jimenez-Donaire, Maria J., Klessen, Ralf S., Koch, Eric W., Liu, Daizhong, Mathur, Smita, Meidt, Sharon, Menon, Shyam H., Neumann, Justus, Pinna, Francesca, Querejeta, Miguel, Sormani, Mattia C., Tress, Robin G.
We study young massive clusters (YMCs) in their embedded "infant" phase with $\sim0.\!^{\prime\prime}1$ ALMA, HST, and JWST observations targeting the central starburst ring in NGC 3351, a nearby Milky Way analog galaxy. Our new ALMA data reveal 18 b
Externí odkaz:
http://arxiv.org/abs/2401.14453
Autor:
Schoedel, Rainer, Longmore, Steve, Henshaw, Jonny, Ginsburg, Adam, Bally, John, Feldmeier, Anja, Hosek, Matt, Lara, Francisco Nogueras, Ciurlo, Anna, Chevance, Mélanie, Kruijssen, J. M. Diederik, Klessen, Ralf, Ponti, Gabriele, Amaro-Seoane, Pau, Anastasopoulou, Konstantina, Anderson, Jay, Arias, Maria, Barnes, Ashley T., Battersby, Cara, Bono, Giuseppe, Ferres, Lucía Bravo, Bryant, Aaron, Gonzáalez, Miguel Cano, Cassisi, Santi, Chaves-Velasquez, Leonardo, Conte, Francesco, Ramos, Rodrigo Contreras, Cotera, Angela, Crowe, Samuel, di Teodoro, Enrico, Do, Tuan, Eisenhauer, Frank, Enokiya, Rei, Fedriani, Rubén, Friske, Jennifer K. S., Gadotti, Dimitri, Gallart, Carme, Calvente, Teresa Gallego, Cano, Eulalia Gallego, Fuentes, Pablo García, Marín, Macarena García, Gardini, Angela, Gautam, Abhimat K., Ghez, Andrea, Gillessen, Stefan, Gouda, Naoteru, Gualandris, Alessia, Guarcello, Mario Giuseppe, Gutermuth, Robert, Haggard, Daryl, Hankins, Matthew, Hu, Yue, Kano, Ryohei, Kauffmann, Jens, Lau, Ryan, Lazarian, Alexandre, Libralato, Mattia, Lu, Anan, Lu, Xing, Lu, Jessica R., Luetzgendorf, Nora, Magorrian, John, Mandel, Shifra, Markoff, Sera, Arranz, Álvaro Martínez, Mastrobuono-Battisti, Alessandra, Melamed, Maria, Mills, Elisabeth, Mori, Kaya, Morris, Mark, Murchikova, Elena, Nagata, Tetsuya, Najarro, Francisco, Nandakumar, Govind, Nataf, David, Neumayer, Nadine, Nishiyama, Shogo, Nobukawa, Masayoshi, Paré, Dylan M, Peissker, Florian, Petkova, Maya, Pillai, Thushara G. S., Román, Mike Rich Carlos, Rugel, Michael, Ryde, Nils, Sabha, Nadeen, Bermúdez, Joel Sánchez, Sánchez-Monge, Álvaro, Schultheis, Mathias, Shao, Lijing, Shinnaga, Hiroko, Simpson, Janet, Takekawa, Shunya, Tan, Jonathan C., Thorsbro, Brian, Torne, Pablo, Tress, Robin Goppala, Uchiyam, Hideki, Valenti, Elena, van der Marel, Roeland, Verberne, Sill, Vermot, Pierre, von Fellenberg, Sebastiano, Walker, Daniel, Witzel, Gunther, Xu, Siyao, Yano, Taihei, Yusef-Zadeh, Farhad, Zajaček, Michal, Zoccali, Manuela
The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post main sequence stars, and the highest volume density of supernovae in the
Externí odkaz:
http://arxiv.org/abs/2310.11912
Autor:
Sormani, Mattia C., Barnes, Ashley T., Sun, Jiayi, Stuber, Sophia K., Schinnerer, Eva, Emsellem, Eric, Leroy, Adam K., Glover, Simon C. O., Henshaw, Jonathan D., Meidt, Sharon E., Neumann, Justus, Querejeta, Miguel, Williams, Thomas G., Bigiel, Frank, Eibensteiner, Cosima, Fragkoudi, Francesca, Levy, Rebecca C., Grasha, Kathryn, Klessen, Ralf S., Kruijssen, J. M. Diederik, Neumayer, Nadine, Pinna, Francesca, Rosolowsky, Erik W., Smith, Rowan J., Teng, Yu-Hsuan, Tress, Robin G., Watkins, Elizabeth J.
Galactic bars can drive cold gas inflows towards the centres of galaxies. The gas transport happens primarily through the so-called bar ``dust lanes'', which connect the galactic disc at kpc scales to the nuclear rings at hundreds of pc scales much l
Externí odkaz:
http://arxiv.org/abs/2305.14437
Autor:
Petkova, Maya A., Kruijssen, J. M. Diederik, Henshaw, Jonathan D., Longmore, Steven N., Glover, Simon C. O., Sormani, Mattia C., Armillotta, Lucia, Barnes, Ashley T., Klessen, Ralf S., Nogueras-Lara, Francisco, Tress, Robin G., Armijos-Abendaño, Jairo, Colzi, Laura, Federrath, Christoph, García, Pablo, Ginsburg, Adam, Henkel, Christian, Martín, Sergio, Riquelme, Denise, Rivilla, Víctor M.
The Central Molecular Zone (CMZ; the central ~ 500 pc of the Galaxy) is a kinematically unusual environment relative to the Galactic disc, with high velocity dispersions and a steep size-linewidth relation of the molecular clouds. In addition, the CM
Externí odkaz:
http://arxiv.org/abs/2304.11190
Autor:
Smith, Rowan J., Tress, Robin, Soler, Juan D., Klessen, Ralf S., Glover, Simon C. O., Hennebelle, Patrick, Molinari, Sergio, Mac Low, Mordecai-Mark, Whitworth, David
The Cold Neutral Medium (CNM) is an important part of the galactic gas cycle and a precondition for the formation of molecular and star forming gas, yet its distribution is still not fully understood. In this work we present extremely high resolution
Externí odkaz:
http://arxiv.org/abs/2301.08265
Autor:
Schinnerer, Eva, Emsellem, Eric, Henshaw, Jonathan D., Liu, Daizhong, Meidt, Sharon E., Querejeta, Miguel, Renaud, Florent, Sormani, Mattia C., Sun, Jiayi, Egorov, Oleg V., Larson, Kirsten L., Leroy, Adam K., Rosolowsky, Erik, Sandstrom, Karin M., Williams, T. G., Barnes, Ashley T., Bigiel, F., Chevance, Melanie, Cao, Yixian, Chandar, Rupali, Dale, Daniel A., Eibensteiner, Cosima, Glover, Simon C. O., Grasha, Kathryn, Hannon, Stephen, Hassani, Hamid, Kim, Jaeyeon, Klessen, Ralf S., Kruijssen, J. M. Diederik, Murphy, Eric J., Neumann, Justus, Pan, Hsi-An, Pety, Jerome, Saito, Toshiki, Stuber, Sophia K., Tress, Robin G., Usero, Antonio, Watkins, Elizabeth J., Whitmore, Bradley C.
Large-scale bars can fuel galaxy centers with molecular gas, often leading to the development of dense ring-like structures where intense star formation occurs, forming a very different environment compared to galactic disks. We pair ~0.3" (30pc) res
Externí odkaz:
http://arxiv.org/abs/2212.09168
Autor:
Lee, Janice C., Sandstrom, Karin M., Leroy, Adam K., Thilker, David A., Schinnerer, Eva, Rosolowsky, Erik, Larson, Kirsten L., Egorov, Oleg V., Williams, Thomas G., Schmidt, Judy, Emsellem, Eric, Anand, Gagandeep S., Barnes, Ashley T., Belfiore, Francesco, Beslic, Ivana, Bigiel, Frank, Blanc, Guillermo A., Bolatto, Alberto D., Boquien, Mederic, Brok, Jakob den, Cao, Yixian, Chandar, Rupali, Chastenet, Jeremy, Chevance, Melanie, Chiang, I-Da, Congiu, Enrico, Dale, Daniel A., Deger, Sinan, Eibensteiner, Cosima, Faesi, Christopher M., Glover, Simon C. O., Grasha, Kathryn, Groves, Brent, Hassani, Hamid, Henny, Kiana F., Henshaw, Jonathan D., Hoyer, Nils, Hughes, Annie, Jeffreson, Sarah, Jimenez-Donaire, Marıa J., Kim, Jaeyeon, Kim, Hwihyun, Klessen, Ralf S., Koch, Eric W., Kreckel, Kathryn, Kruijssen, J. M. Diederik, Li, Jing, Liu, Daizhong, Lopez, Laura A., Maschmann, Daniel, Chen, Ness Mayker, Meidt, Sharon E., Murphy, Eric J., Neumann, Justus, Neumayer, Nadine, Pan, Hsi-An, Pessa, Ismael, Pety, Jerome, Querejeta, Miguel, Pinna, Francesca, Rodrıguez, M. Jimena, Saito, Toshiki, Sanchez-Blazquez, Patricia, Santoro, Francesco, Sardone, Amy, Smith, Rowan J., Sormani, Mattia C., Scheuermann, Fabian, Stuber, Sophia K., Sutter, Jessica, Sun, Jiayi, Teng, Yu-Hsuan, Tress, Robin G., Usero, Antonio, Watkins, Elizabeth J., Whitmore, Bradley C., Razza, Alessandro
The PHANGS collaboration has been building a reference dataset for the multi-scale, multi-phase study of star formation and the interstellar medium in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-resol
Externí odkaz:
http://arxiv.org/abs/2212.02667