Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Stuber, Sophia K"'
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:
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:
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
Surveying the Whirlpool at Arcseconds with NOEMA (SWAN)- I. Mapping the HCN and N$_2$H$^+$ 3mm lines
Autor:
Stuber, Sophia K., Pety, Jerome, Schinnerer, Eva, Bigiel, Frank, Usero, Antonio, Beslić, Ivana, Querejeta, Miguel, Jiménez-Donaire, María J., Leroy, Adam, Brok, Jakob den, Neumann, Lukas, Eibensteiner, Cosima, Teng, Yu-Hsuan, Barnes, Ashley, Chevance, Mélanie, Colombo, Dario, Dale, Daniel A., Glover, Simon C. O., Liu, Daizhong, Pan, Hsi-An
We present the first results from "Surveying the Whirlpool at Arcseconds with NOEMA" (SWAN), an IRAM Northern Extended Millimetre Array (NOEMA)+30m large program that maps emission from several molecular lines at 90 and 110 GHz in the iconic nearby g
Externí odkaz:
http://arxiv.org/abs/2312.09810
Autor:
Teng, Yu-Hsuan, Chiang, I-Da, Sandstrom, Karin M., Sun, Jiayi, Leroy, Adam K., Bolatto, Alberto D., Usero, Antonio, Ostriker, Eve C., Querejeta, Miguel, Chastenet, Jeremy, Bigiel, Frank, Boquien, Mederic, Brok, Jakob den, Cao, Yixian, Chevance, Melanie, Chown, Ryan, Colombo, Dario, Eibensteiner, Cosima, Glover, Simon C. O., Grasha, Kathryn, Henshaw, Jonathan D., Jimenez-Donaire, Maria J., Liu, Daizhong, Murphy, Eric J., Pan, Hsi-An, Stuber, Sophia K., Williams, Thomas G.
Determining how galactic environment, especially the high gas densities and complex dynamics in bar-fed galaxy centers, alters the star formation efficiency (SFE) of molecular gas is critical to understanding galaxy evolution. However, these same phy
Externí odkaz:
http://arxiv.org/abs/2310.16037
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:
Liu, Daizhong, Schinnerer, Eva, Cao, Yixian, Leroy, Adam, Usero, Antonio, Rosolowsky, Erik, Emsellem, Eric, Kruijssen, J. M. Diederik, Chevance, Mélanie, Glover, Simon C. O., Sormani, Mattia C., Bolatto, Alberto D., Sun, Jiayi, Stuber, Sophia K., Teng, Yu-Hsuan, Bigiel, Frank, Bešlić, Ivana, Grasha, Kathryn, Henshaw, Jonathan D., Barnes, Ashley. T., Brok, Jakob S. den, Saito, Toshiki, Dale, Daniel A., Watkins, Elizabeth J., Pan, Hsi-An, Klessen, Ralf S., Anand, Gagandeep S., Deger, Sinan, Egorov, Oleg V., Faesi, Christopher M., Hassani, Hamid, Larson, Kirsten L., Lee, Janice C., Lopez, Laura A., Pety, Jérôme, Sandstrom, Karin, Thilker, David A., Whitmore, Bradley C., Williams, Thomas G.
We compare embedded young massive star clusters (YMCs) to (sub-)millimeter line observations tracing the excitation and dissociation of molecular gas in the starburst ring of NGC 1365. This galaxy hosts one of the strongest nuclear starbursts and ric
Externí odkaz:
http://arxiv.org/abs/2212.09652
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