Zobrazeno 1 - 10
of 274
pro vyhledávání: '"Smith, Matthew W."'
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
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:
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:
Vieira, Helena Faustino, Duarte-Cabral, Ana, Davis, Timothy A., Peretto, Nicolas, Smith, Matthew W. L., Querejeta, Miguel, Colombo, Dario, Anderson, Michael
Here we present the cloud population extracted from M51, following the application of our new high-resolution dust extinction technique to the galaxy (Faustino Vieira et al. 2023). With this technique, we are able to image the gas content of the enti
Externí odkaz:
http://arxiv.org/abs/2310.18210
Autor:
Vieira, Helena Faustino, Duarte-Cabral, Ana, Davis, Timothy A., Peretto, Nicolas, Smith, Matthew W. L., Querejeta, Miguel, Colombo, Dario, Anderson, Michael
We present a new dust extinction technique with which we are able to retrieve parsec-scale gas surface density maps for entire nearby galaxies. The method measures the dust attenuation in optical bands on a pixel-by-pixel basis against a smoothed, re
Externí odkaz:
http://arxiv.org/abs/2306.11508
Autor:
Loni, Alessandro, Serra, Paolo, Sarzi, Marc, Józsa, Gyula I. G., Anta, Pablo M. Galán-de, Zabel, Nikki, Kleiner, Dane, Maccagni, Filippo M., Molnár, Daniel, Ramatsoku, Mpati, Loi, Francesca, Corsini, Enrico M., Pisano, D. J., Kamphuis, Peter, Davis, Timothy A., de Blok, W. J. G., Dettmar, Ralf J., Falcon-Barroso, Jesus, Iodice, Enrichetta, Lara-López, Maritza A., Loubser, S. Ilani, Morokuma-Matsui, Kana, Peletier, Reynier, Pinna, Francesca, Poci, Adriano, Smith, Matthew W. L., Trager, Scott C., van de Ven, Glenn
We study the evolutionary path of the Fornax cluster galaxy NGC$~$1436, which is known to be currently transitioning from a spiral into a lenticular morphology. This galaxy hosts an inner star-forming disc and an outer quiescent disc, and we analyse
Externí odkaz:
http://arxiv.org/abs/2305.05709
We have measured the mass of metals in the molecular gas in 13 submillimetre galaxies at z~4 in which the gas, based on previous observations, lies in a cold rotating disk. We measured the metal masses using either the submillimetre line or continuum
Externí odkaz:
http://arxiv.org/abs/2303.07376
Autor:
Clark, Christopher J. R., Roman-Duval, Julia C., Gordon, Karl D., Bot, Caroline, Smith, Matthew W. L., Hagen, Lea M. Z.
We explore evolution in the dust-to-gas ratio with density within four well-resolved Local Group galaxies - the LMC, SMC, M31, and M33. We do this using new ${\it Herschel}$ maps, which restore extended emission that was missed by previous ${\it Hers
Externí odkaz:
http://arxiv.org/abs/2302.07378
Autor:
Chown, Ryan, Parker, Laura C., Wilson, Christine D., Brown, Toby, Evans, Fraser A., Gao, Yang, Hwang, Ho Seong, Lin, Lihwai, Saintonge, Amelie, Sargent, Mark, Smith, Matthew W. L., Xiao, Ting
We study the cold gas and dust properties for a sample of red star forming galaxies called "red misfits." We collect single-dish CO observations and HI observations from representative samples of low-redshift galaxies, as well as our own JCMT CO obse
Externí odkaz:
http://arxiv.org/abs/2208.03842
Autor:
Smith, Matthew W. L., Eales, Stephen A., Williams, Thomas G., Lee, Bumhyun, Li, Zongnan, Barmby, Pauline, Bureau, Martin, Chapman, Scott, Cho, Brian S., Chung, Aeree, Chung, Eun Jung, Chung, Hui-Hsuan, Clark, Christopher J. R., Clements, David L., Davis, Timothy A., De Looze, Ilse, Eden, David J., Athikkat-Eknath, Gayathri, Ford, George P., Gao, Yu, Gear, Walter, Gomez, Haley L., de Grijs, Richard, He, Jinhua, Ho, Luis C., Hughes, Thomas M., Jiao, Sihan, Li, Zhiyuan, Kemper, Francisca, Kirchschlager, Florian, Koch, Eric W., Kong, Albert K. H., Lee, Chien-Hsiu, Lin, En-Tzu, Mairs, Steve, Michalowski, Michal J., Pattle, Kate, Peng, Yingjie, Ragan, Sarah E., Rawlings, Mark G., Rigopoulou, Dimitra, Saintonge, Amelie, Schruba, Andreas, Tang, Xindi, Wang, Junfeng, Whitworth, Anthony P., Wilson, Christine D., Yim, Kijeong, Zhu, Ming
Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths compared to the brightness at the peak of the dust emission. Second, it i
Externí odkaz:
http://arxiv.org/abs/2110.00011