Zobrazeno 1 - 10
of 213
pro vyhledávání: '"Saintonge, Amelie"'
Autor:
Chamba, Nushkia, Marcum, Pamela M., Saintonge, Amélie, Borlaff, Alejandro S., Hayes, Matthew J., Gouellec, Valentin J. M. Le, Chojnowski, S. Drew, Fanelli, Michael N.
Mapping stars and gas in nearby galaxies is fundamental for understanding their growth and the impact of their environment. This issue is addressed by comparing the stellar "edges" of galaxies $D_{\rm stellar}$, defined as the outermost diameter wher
Externí odkaz:
http://arxiv.org/abs/2408.13311
Autor:
Chastenet, Jérémy, De Looze, Ilse, Relaño, Monica, Dale, Daniel A., Williams, Thomas G., Bianchi, Simone, Xilouris, Emmanuel M., Baes, Maarten, Bolatto, Alberto D., Boyer, Martha L., Casasola, Viviana, Clark, Christopher J. R., Fraternali, Filippo, Fritz, Jacopo, Galliano, Frédéric, Glover, Simon C. O., Gordon, Karl D., Hirashita, Hiroyuki, Kennicutt, Robert, Nagamine, Kentaro, Kirchschlager, Florian, Klessen, Ralf S., Koch, Eric W., Levy, Rebecca C., McCallum, Lewis, Madden, Suzanne C., McLeod, Anna F., Meidt, Sharon E., Mosenkov, Aleksandr V., Richie, Helena M., Saintonge, Amélie, Sandstrom, Karin M., Schneider, Evan E., Sivkova, Evgenia E., Smith, J. D. T., Smith, Matthew W. L., van der Wel, Arjen, Walch, Stefanie, Walter, Fabian, Wood, Kenneth
Publikováno v:
A&A 690, A348 (2024)
We present new JWST observations of the nearby, prototypical edge-on, spiral galaxy NGC 891. The northern half of the disk was observed with NIRCam in its F150W and F277W filters. Absorption is clearly visible in the mid-plane of the F150W image, alo
Externí odkaz:
http://arxiv.org/abs/2408.08026
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:
Booth, Mark, Klaassen, Pamela, Cicone, Claudia, Mroczkowski, Tony, Wedemeyer, Sven, Akiyama, Kazunori, Bower, Geoffrey, Cordiner, Martin A., Di Mascolo, Luca, Johnstone, Doug, van Kampen, Eelco, Lee, Minju M., Liu, Daizhong, Orlowski-Scherer, John, Saintonge, Amélie, Smith, Matthew, Thelen, Alexander E.
Sub-mm and mm 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 brightest (sub-)mm so
Externí odkaz:
http://arxiv.org/abs/2405.20140
Star formation histories (SFHs) of galaxies are affected by a variety of factors, both external (field vs. cluster/group) and internal (presence of a bar and AGN, morphological type). In this work, we extend our previous study and apply the /
Externí odkaz:
http://arxiv.org/abs/2404.19473
Autor:
Orlowski-Scherer, John, Maccarone, Thomas J., Bright, Joe, Kaminski, Tomasz, Koss, Michael, Mohan, Atul, Montenegro-Montes, Francisco Miguel, Næss, Sig urd, Ricci, Claudio, Severgnini, Paola, Stanke, Thomas, Vignali, Cristian, Wedemeyer, Sven, Booth, Mark, Cicone, Claudia, Di Mascolo, Luca, Johnstone, Doug, Mroczkowski, Tony, Cordiner, Martin A., Greiner, Jochen, Hatziminaoglou, Evanthia, van Kampen, Eelco, Klaassen, Pamela, Lee, Minju M., Liu, Daizhong, Saintonge, Amelie, Smith, Matthew, Thelen, Alexander E.
The study of transient and variable events, including novae, active galactic nuclei, and black hole binaries, has historically been a fruitful path for elucidating the evolutionary mechanisms of our universe. The study of such events in the millimete
Externí odkaz:
http://arxiv.org/abs/2404.13133
Autor:
van Kampen, Eelco, Bakx, Tom, De Breuck, Carlos, Chen, Chian-Chou, Dannerbauer, Helmut, Magnelli, Benjamin, Montenegro-Montes, Francisco Miguel, Okumura, Teppei, Pu, Sy-Yun, Rybak, Matus, Saintonge, Amelie, Cicone, Claudia, Hatziminaoglou, Evanthia, Hilhorst, Juliette, Klaassen, Pamela, Lee, Minju, Lovell, Christopher C., Lundgren, Andreas, Di Mascolo, Luca, Mroczkowski, Tony, Sommovigo, Laura, Booth, Mark, Cordiner, Martin A., Ivison, Rob, Johnstone, Doug, Liu, Daizhong, Maccarone, Thomas J., Smith, Matthew, Thelen, Alexander E., Wedemeyer, Sven
During the most active period of star formation in galaxies, which occurs in the redshift range 1
Externí odkaz:
http://arxiv.org/abs/2403.02806
Autor:
Cordiner, Martin A., Thelen, Alexander E., Cavalié, Thibault, Cosentino, Richard, Fletcher, Leigh N., Gurwell, Mark, de Kleer, Katherine, Kuan, Yi-Jehng, Lellouch, Emmanuel, Moullet, Arielle, Nixon, Conor, de Pater, Imke, Teanby, Nicholas A., Butler, Bryan, Charnley, Steven, Moreno, Raphael, Booth, Mark, Klaassen, Pamela, Cicone, Claudia, Mroczkowski, Tony, Di Mascolo, Luca, Johnstone, Doug, van Kampen, Eelco, Lee, Minju M., Liu, Daizhong, Maccarone, Thomas J., Saintonge, Amélie, Smith, Matthew, Wedemeyer, Sven
The study of planets and small bodies within our Solar System is fundamental for understanding the formation and evolution the Earth and other planets. Compositional and meteorological studies of the giant planets provide a foundation for understandi
Externí odkaz:
http://arxiv.org/abs/2403.02258
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