Zobrazeno 1 - 10
of 2 794
pro vyhledávání: '"Stuber, A. P."'
Autor:
Brok, Jakob den, Jiménez-Donaire, María J., Leroy, Adam, Schinnerer, Eva, Bigiel, Frank, Pety, Jérôme, Petitpas, Glen, Usero, Antonio, Teng, Yu-Hsuan, Humire, Pedro, Koch, Eric W., Rosolowsky, Erik, Sandstrom, Karin, Liu, Daizhong, Zhang, Qizhou, Stuber, Sophia, Chevance, Mélanie, Dale, Daniel A., Eibensteiner, Cosima, Galić, Ina, Glover, Simon C. O., Pan, Hsi-An, Querejeta, Miguel, Smith, Rowan J., Williams, Thomas G., Wilner, David J., Zhang, Valencia
Over the past decade, several millimeter interferometer programs have mapped the nearby star-forming galaxy M51 at a spatial resolution of ${\le}170$ pc. This study combines observations from three major programs: the PdBI Arcsecond Whirlpool Survey
Externí odkaz:
http://arxiv.org/abs/2410.21399
Autor:
Ruiz-García, Marina, Querejeta, Miguel, García-Burillo, Santiago, Emsellem, Eric, Meidt, Sharon E., Sormani, Mattia C., Schinnerer, Eva, Williams, Thomas G., Bazzi, Zein, Colombo, Dario, Gleis, Damian R., Gnedin, Oleg Y., Klessen, Ralf S., Leroy, Adam K., Sánchez-Blázquez, Patricia, Stuber, Sophia K.
Bars are remarkable stellar structures that can transport gas toward centers and drive the secular evolution of galaxies. In this context, it is important to locate dynamical resonances associated with bars. For this study, we used ${Spitzer}$ near-i
Externí odkaz:
http://arxiv.org/abs/2410.13353
Autor:
Neumann, Justus, Thomas, Daniel, Maraston, Claudia, Gleis, Damian R., Mao, Chuanming, Schinnerer, Eva, Stuber, Sophia K.
Bars are expected to impact the distribution of stellar populations both during bar formation, as they rearrange stars into new orbits, and afterwards, due to the redistribution of star-formation-fuelling gas and transfer of angular momentum. We stud
Externí odkaz:
http://arxiv.org/abs/2409.18180
Autor:
Laudage, Sebastian, Eibensteiner, Cosima, Bigiel, Frank, Leroy, Adam K., Meidt, Sharon, Schinnerer, Eva, de Blok, W. J. G., Querejeta, Miguele, Stuber, Sophia, Colombo, Dario, Rosolowsky, Erik, Pisano, D. J., Utomo, Dyas, Levy, Rebecca C., Klessen, Ralf, Cao, Yixian, Koch, Eric W., Kurapati, Sushma, Sanchez-Blazquez, Patricia, Neumann, Justus, Neumann, Lukas, Pan, Hsi-An, Williams, Thomas G.
Publikováno v:
A&A 690, A169 (2024)
Neutral atomic gas (HI) effectively traces galactic dynamics across mid to large galactocentric radii. However, its limitations in observing small-scale changes within the central few kiloparsecs, coupled with the often observed HI deficit in galacti
Externí odkaz:
http://arxiv.org/abs/2407.04531
Autor:
Giacchi, Gianluca, Iakovidis, Isidoros, Milani, Bastien, Stuber, Matthias, Murray, Micah, Franceschiello, Benedetta
Magnetic Resonance Imaging (MRI) is a powerful technique employed for non-invasive in vivo visualization of internal structures. Sparsity is often deployed to accelerate the signal acquisition or overcome the presence of motion artifacts, improving t
Externí odkaz:
http://arxiv.org/abs/2406.19239
Autor:
Neumann, Lukas, Bigiel, Frank, Barnes, Ashley T., Gallagher, Molly J., Leroy, Adam, Usero, Antonio, Rosolowsky, Erik, Bešlić, Ivana, Boquien, Médéric, Cao, Yixian, Chevance, Mélanie, Colombo, Dario, Dale, Daniel A., Eibensteiner, Cosima, Grasha, Kathryn, Henshaw, Jonathan D., Jiménez-Donaire, María J., Meidt, Sharon, Menon, Shyam H., Murphy, Eric J., Pan, Hsi-An, Querejeta, Miguel, Saito, Toshiki, Schinnerer, Eva, Stuber, Sophia K., Teng, Yu-Hsuan, Williams, Thomas G.
Publikováno v:
A&A 691, A121 (2024)
The star formation rate (SFR) is tightly connected to the amount of dense gas in molecular clouds. However, it is not fully understood how the relationship between dense molecular gas and star formation varies within galaxies and in different morphol
Externí odkaz:
http://arxiv.org/abs/2406.12025
Autor:
Querejeta, Miguel, Leroy, Adam K., Meidt, Sharon E., Schinnerer, Eva, Belfiore, Francesco, Emsellem, Eric, Klessen, Ralf S., Sun, Jiayi, Sormani, Mattia, Bešlic, Ivana, Cao, Yixian, Chevance, Mélanie, Colombo, Dario, Dale, Daniel A., García-Burillo, Santiago, Glover, Simon C. O., Grasha, Kathryn, Groves, Brent, Koch, Eric. W., Neumann, Lukas, Pan, Hsi-An, Pessa, Ismael, Pety, Jérôme, Pinna, Francesca, Ramambason, Lise, Razza, Alessandro, Romanelli, Andrea, Rosolowsky, Erik, Ruiz-García, Marina, Sánchez-Blázquez, Patricia, Smith, Rowan, Stuber, Sophia, Ubeda, Leonardo, Usero, Antonio, Williams, Thomas G.
Spiral arms are some of the most spectacular features in disc galaxies, and also present in our own Milky Way. It has been argued that star formation should proceed more efficiently in spiral arms as a result of gas compression. Yet, observational st
Externí odkaz:
http://arxiv.org/abs/2405.05364
Autor:
Douaki, Ali, Weng, Shukun, Lanzavecchia, German, Sapunova, Anastasiia, Stuber, Annina, Nanni, Gabriele, Nakatsuka, Nako, Tsutsui, Makusu, Yokota, Kazumichi, Krahne, Roman, Garoli, Denis
Solid-state nanopore gating inspired by biological ion channels is gaining increasing traction due to a large range of applications in biosensing and drug delivery. Integration of stimuli-responsive molecules such as poly(N-isopropylacrylamide) (PNIP
Externí odkaz:
http://arxiv.org/abs/2405.02894
Autor:
Yamamoto, Takashi, Iono, Daisuke, Saito, Toshiki, Kuno, Nario, Stuber, Sophia K., Liu, Daizhong, Williams, Thomas G.
We present a quantitative and statistical analysis of the molecular gas morphology in 73 nearby galaxies using high spatial resolution CO (J=2-1) data obtained from the Atacama Large Millimeter/submillimeter Array (ALMA) by the PHANGS large program.
Externí odkaz:
http://arxiv.org/abs/2404.01427
Autor:
Williams, Thomas G., Lee, Janice C., Larson, Kirsten L., Leroy, Adam K., Sandstrom, Karin, Schinnerer, Eva, Thilker, David A., Belfiore, Francesco, Egorov, Oleg V., Rosolowsky, Erik, Sutter, Jessica, DePasquale, Joseph, Pagan, Alyssa, Berger, Travis A., Anand, Gagandeep S., Barnes, Ashley T., Bigiel, Frank, Boquien, Médéric, Cao, Yixian, Chastenet, Jérémy, Chevance, Mélanie, Chown, Ryan, Dale, Daniel A., Deger, Sinan, Eibensteiner, Cosima, Emsellem, Eric, Faesi, Christopher M., Glover, Simon C. O., Grasha, Kathryn, Hannon, Stephen, Hassani, Hamid, Henshaw, Jonathan D., Jiménez-Donaire, María J., Kim, Jaeyeon, Klessen, Ralf S., Koch, Eric W., Li, Jing, Liu, Daizhong, Meidt, Sharon E., Méndez-Delgado, J. Eduardo, Murphy, Eric J., Neumann, Justus, Neumann, Lukas, Neumayer, Nadine, Oakes, Elias K., Pathak, Debosmita, Pety, Jérôme, Pinna, Francesca, Querejeta, Miguel, Ramambason, Lise, Romanelli, Andrea, Sormani, Mattia C., Stuber, Sophia K., Sun, Jiayi, Teng, Yu-Hsuan, Usero, Antonio, Watkins, Elizabeth J., Weinbeck, Tony D.
The exquisite angular resolution and sensitivity of JWST is opening a new window for our understanding of the Universe. In nearby galaxies, JWST observations are revolutionizing our understanding of the first phases of star formation and the dusty in
Externí odkaz:
http://arxiv.org/abs/2401.15142