Zobrazeno 1 - 10
of 608
pro vyhledávání: '"Teuben, P."'
Autor:
Lenkić, Laura, Fisher, Deanne B., Bolatto, Alberto D., Teuben, Peter J., Levy, Rebecca C., Sun, Jiayi, Herrera-Camus, Rodrigo, Glazebrook, Karl, Obreschkow, Danail, Abraham, Roberto
The gas-phase velocity dispersions in disk galaxies, which trace turbulence in the interstellar medium, are observed to increase with lookback time. However, the mechanisms that set this rise in turbulence are observationally poorly constrained. To a
Externí odkaz:
http://arxiv.org/abs/2408.02730
Autor:
Wong, Tony, Cao, Yixian, Luo, Yufeng, Bolatto, Alberto D., Sánchez, Sebastián F., Barrera-Ballesteros, Jorge K., Blitz, Leo, Colombo, Dario, Dannerbauer, Helmut, Green, Alex, Kalinova, Veselina, Khan, Ferzem, Kim, Andrew, Lacerda, Eduardo A. D., Leroy, Adam K., Levy, Rebecca C., Lin, Xincheng, Luo, Yuanze, Rosolowsky, Erik W., Rubio, Mónica, Teuben, Peter, Utomo, Dyas, Villanueva, Vicente, Vogel, Stuart N., Wang, Xinyu
The EDGE-CALIFA survey provides spatially resolved optical integral field unit (IFU) and CO spectroscopy for 125 galaxies selected from the CALIFA Data Release 3 sample. The Extragalactic Database for Galaxy Evolution (EDGE) presents the spatially re
Externí odkaz:
http://arxiv.org/abs/2401.13181
Autor:
Villanueva, Vicente, Bolatto, Alberto D., Vogel, Stuart N., Wong, Tony, Leroy, Adam K., Sanchez, Sebastian F., Levy, Rebecca C., Rosolowsky, Erik, Colombo, Dario, Kalinova, Veselina, Cronin, Serena, Teuben, Peter, Rubio, Monica, Bazzi, Zein
We present a $^{12}$CO($J$=2-1) survey of 60 local galaxies using data from the Atacama Large Millimeter/submillimeter Compact Array as part of the Extragalactic Database for Galaxy Evolution: the ACA EDGE survey. These galaxies all have integral fie
Externí odkaz:
http://arxiv.org/abs/2312.03995
Autor:
Blanton, Michael R., Evans, Janet D., Norman, Dara, O'Mullane, William, Price-Whelan, Adrian, Rizzi, Luca, Accomazzi, Alberto, Ansdell, Megan, Bailey, Stephen, Barrett, Paul, Berukoff, Steven, Bolton, Adam, Borrill, Julian, Cruz, Kelle, Dalcanton, Julianne, Desai, Vandana, Dubois-Felsmann, Gregory P., Economou, Frossie, Ferguson, Henry, Field, Bryan, Foreman-Mackey, Dan, Forero-Romero, Jaime, Gaffney, Niall, Gillies, Kim, Graham, Matthew J., Gwyn, Steven, Hennawi, Joseph, Hughes, Anna L. H., Jaffe, Tess, Jagannathan, Preshanth, Jenness, Tim, Jurić, Mario, Kavelaars, JJ, Kee, Kerk, Kern, Jeff, Kremin, Anthony, Labrie, Kathleen, Lacy, Mark, Law, Casey, Martínez-Galarza, Rafael, McCully, Curtis, McEnery, Julie, Miller, Bryan, Moriarty, Christopher, Muench, August, Muna, Demitri, Murillo, Angela, Narayan, Gautham, Neill, James D., Nikutta, Robert, Ojha, Roopesh, Olsen, Knut, O'Meara, John, Rusholme, Ben, Seaman, Robert, Starkman, Nathaniel, Still, Martin, Stoehr, Felix, Swinbank, John D., Teuben, Peter, Toledo, Ignacio, Tollerud, Erik, Turk, Matthew D., Turner, James, Vacca, William, Vieira, Joaquin, Weaver, Benjamin, Weiner, Benjamin, Weiss, Jason, Westfall, Kyle, Willman, Beth, Zhao, Lily
The astronomical community is grappling with the increasing volume and complexity of data produced by modern telescopes, due to difficulties in reducing, accessing, analyzing, and combining archives of data. To address this challenge, we propose the
Externí odkaz:
http://arxiv.org/abs/2311.04272
Autor:
Plunkett, Adele, Hacar, Alvaro, Moser-Fischer, Lydia, Petry, Dirk, Teuben, Peter, Pingel, Nickolas, Kunneriath, Devaky, Takagi, Toshinobu, Miyamoto, Yusuke, Moravec, Emily, Suri, Sumeyye, Hess, Kelley M., Hoffman, Melissa, Mason, Brian
Modern interferometers routinely provide radio-astronomical images down to subarcsecond resolution. However, interferometers filter out spatial scales larger than those sampled by the shortest baselines, which affects the measurement of both spatial
Externí odkaz:
http://arxiv.org/abs/2303.02177
Autor:
Yu, Si-Yue, Kalinova, Veselina, Colombo, Dario, Bolatto, Alberto D., Wong, Tony, Levy, Rebecca C., Villanueva, Vicente, Sánchez, Sebastián F., Ho, Luis C., Vogel, Stuart N., Teuben, Peter, Rubio, Mónica
Publikováno v:
A&A 666, A175 (2022)
Shocks and torques produced by non-axisymmetric structures such as spiral arms and bars may transport gas to galaxy central regions. We test this hypothesis by studying the dependence of concentration of CO luminosity ($C_{CO}$), molecular gas ($C_{m
Externí odkaz:
http://arxiv.org/abs/2208.14950
Autor:
Levy, Rebecca C., Bolatto, Alberto D., Leroy, Adam K., Sormani, Mattia C., Emig, Kimberly L., Gorski, Mark, Lenkić, Laura, Mills, Elisabeth A. C., Tarantino, Elizabeth, Teuben, Peter, Veilleux, Sylvain, Walter, Fabian
The center of the nearby galaxy NGC\,253 hosts a population of more than a dozen super star clusters (SSCs) which are still in the process of forming. The majority of the star formation of the burst is concentrated in these SSCs, and the starburst is
Externí odkaz:
http://arxiv.org/abs/2206.04700
Autor:
Emig, K. L., White, G. J., Salas, P., Karim, R. L., van Weeren, R. J., Teuben, P. J., Zavagno, A., Chiu, P., Haverkorn, M., Oonk, J. B. R., Orrú, E., Polderman, I. M., Reich, W., Röttgering, H. J. A., Tielens, A. G. G. M.
Publikováno v:
A&A 664, A88 (2022)
Ionized gas probes the influence of massive stars on their environment. The Cygnus X region (d~1.5 kpc) is one of the most massive star forming complexes in our Galaxy, in which the Cyg OB2 association (age of 3-5 Myr and stellar mass $2 \times 10^{4
Externí odkaz:
http://arxiv.org/abs/2205.09193
Autor:
Heyer, Mark, Gregg, Benjamin, Calzetti, Daniela, Elmegreen, Bruce G., Kennicutt, Robert, Adamo, Angela, Evans, Aaron S., Grasha, Kathryn, Lowenthal, James D., Narayanan, Gopal, Rosa-Gonzalez, Daniel, Schloerb, F. P., Souccar, Kamal, Tang, Yuping, Teuben, Peter, Vega, Olga, Wall, William F., Yun, Min S.
Observations of 12CO J=1-0 and HCN J=1-0 emission from NGC 5194 (M51) made with the 50~meter Large Millimeter Telescope and the SEQUOIA focal plane array are presented. Using the HCN to CO ratio, we examine the dense gas mass fraction over a range of
Externí odkaz:
http://arxiv.org/abs/2204.09613
Autor:
Engel, Kristi, Lewis, Tiffany, Muzio, Marco Stein, Venters, Tonia M., Ahlers, Markus, Albert, Andrea, Allen, Alice, Solares, Hugo Alberto Ayala, Anandagoda, Samalka, Andersen, Thomas, Antier, Sarah, Alvarez-Castillo, David, Bar, Olaf, Beznosko, Dmitri, Bibrzyck, Łukasz, Brazier, Adam, Brisbois, Chad, Brose, Robert, Brown, Duncan A., Bulla, Mattia, Burgess, J. Michael, Burns, Eric, Chirenti, Cecilia, Ciprini, Stefano, Clay, Roger, Coughlin, Michael W., Cummings, Austin, D'Elia, Valerio, Dai, Shi, Dietrich, Tim, Di Lalla, Niccolò, Dingus, Brenda, Durocher, Mora, Eser, Johannes, Filipović, Miroslav D., Fleischhack, Henrike, Foucart, Francois, Frontczak, Michał, Fryer, Christopher L., Gamble, Ronald S., Gasparrini, Dario, Giardino, Marco, Goodman, Jordan, Harding, J. Patrick, Hare, Jeremy, Holley-Bockelmann, Kelly, Homola, Piotr, Hughes, Kaeli A., Humensky, Brian, Inoue, Yoshiyuki, Jaffe, Tess, Kargaltsev, Oleg, Kierans, Carolyn, Kneller, James P., Leto, Cristina, Lucarelli, Fabrizio, Martínez-Huerta, Humberto, Maselli, Alessandro, Meli, Athina, Meyers, Patrick, Mueller, Guido, Nasipak, Zachary, Negro, Michela, Niedźwiecki, Michał, Noble, Scott C., Omodei, Nicola, Oslowski, Stefan, Perri, Matteo, Piekarczyk, Marcin, Pittori, Carlotta, Polenta, Gianluca, Prechelt, Remy L., Principe, Giacomo, Racusin, Judith, Rzecki, Krzysztof, Sambruna, Rita M., Schlieder, Joshua E., Shoemaker, David, Smale, Alan, Sośnicki, Tomasz, Stein, Robert, Stuglik, Sławomir, Teuben, Peter, Thorpe, James Ira, Verbiest, Joris P., Verrecchia, Franceso, Vitale, Salvatore, Wadiasingh, Zorawar, Wibig, Tadeusz, Willox, Elijah, Wilson-Hodge, Colleen A., Wood, Joshua, Yang, Hui, Zhang, Haocheng
The last decade has brought about a profound transformation in multimessenger science. Ten years ago, facilities had been built or were under construction that would eventually discover the nature of objects in our universe could be detected through
Externí odkaz:
http://arxiv.org/abs/2203.10074