Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Robin G. Tress"'
Autor:
Jiayi Sun, Hao He, Kyle Batschkun, Rebecca C. Levy, Kimberly Emig, M. Jimena Rodríguez, Hamid Hassani, Adam K. Leroy, Eva Schinnerer, Eve C. Ostriker, Christine D. Wilson, Alberto D. Bolatto, Elisabeth A. C. Mills, Erik Rosolowsky, Janice C. Lee, Daniel A. Dale, Kirsten L. Larson, David A. Thilker, Leonardo Ubeda, Bradley C. Whitmore, Thomas G. Williams, Ashley T. Barnes, Frank Bigiel, Mélanie Chevance, Simon C. O. Glover, Kathryn Grasha, Brent Groves, Jonathan D. Henshaw, Rémy Indebetouw, María J. Jiménez-Donaire, Ralf S. Klessen, Eric W. Koch, Daizhong Liu, Smita Mathur, Sharon Meidt, Shyam H. Menon, Justus Neumann, Francesca Pinna, Miguel Querejeta, Mattia C. Sormani, Robin G. Tress
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 2, p 133 (2024)
We use 0.1″ observations from the Atacama Large Millimeter Array (ALMA), Hubble Space Telescope (HST), and JWST to study young massive clusters (YMCs) in their embedded “infant” phase across the central starburst ring in NGC 3351. Our new ALMA
Externí odkaz:
https://doaj.org/article/dae0cfc139de4f4fb8817c4e0c898348
Autor:
Janice C. Lee, Karin M. Sandstrom, Adam K. Leroy, David A. Thilker, Eva Schinnerer, Erik Rosolowsky, Kirsten L. Larson, Oleg V. Egorov, Thomas G. Williams, Judy Schmidt, Eric Emsellem, Gagandeep S. Anand, Ashley T. Barnes, Francesco Belfiore, Ivana Bešlić, Frank Bigiel, Guillermo A. Blanc, Alberto D. Bolatto, Médéric Boquien, Jakob den Brok, Yixian Cao, Rupali Chandar, Jérémy Chastenet, Mélanie Chevance, I-Da Chiang, Enrico Congiu, Daniel A. Dale, Sinan Deger, Cosima Eibensteiner, Christopher M. Faesi, Simon C. O. Glover, Kathryn Grasha, Brent Groves, Hamid Hassani, Kiana F. Henny, Jonathan D. Henshaw, Nils Hoyer, Annie Hughes, Sarah Jeffreson, María J. Jiménez-Donaire, Jaeyeon Kim, Hwihyun Kim, Ralf S. Klessen, Eric W. Koch, Kathryn Kreckel, J. M. Diederik Kruijssen, Jing Li, Daizhong Liu, Laura A. Lopez, Daniel Maschmann, Ness Mayker Chen, Sharon E. Meidt, Eric J. Murphy, Justus Neumann, Nadine Neumayer, Hsi-An Pan, Ismael Pessa, Jérôme Pety, Miguel Querejeta, Francesca Pinna, M. Jimena Rodríguez, Toshiki Saito, Patricia Sánchez-Blázquez, Francesco Santoro, Amy Sardone, Rowan J. Smith, Mattia C. Sormani, Fabian Scheuermann, Sophia K. Stuber, Jessica Sutter, Jiayi Sun, Yu-Hsuan Teng, Robin G. Treß, Antonio Usero, Elizabeth J. Watkins, Bradley C. Whitmore, Alessandro Razza
Publikováno v:
The Astrophysical Journal Letters, Vol 944, Iss 2, p L17 (2023)
The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-
Externí odkaz:
https://doaj.org/article/f8f700840a4c4803a5cfc64e968e6651
Autor:
Ashley. T. Barnes, Elizabeth J. Watkins, Sharon E. Meidt, Kathryn Kreckel, Mattia C. Sormani, Robin G. Treß, Simon C. O. Glover, Frank Bigiel, Rupali Chandar, Eric Emsellem, Janice C. Lee, Adam K. Leroy, Karin M. Sandstrom, Eva Schinnerer, Erik Rosolowsky, Francesco Belfiore, Guillermo A. Blanc, Médéric Boquien, Jakob den Brok, Yixian Cao, Mélanie Chevance, Daniel A. Dale, Oleg V. Egorov, Cosima Eibensteiner, Kathryn Grasha, Brent Groves, Hamid Hassani, Jonathan D. Henshaw, Sarah Jeffreson, María J. Jiménez-Donaire, Benjamin W. Keller, Ralf S. Klessen, Eric W. Koch, J. M. Diederik Kruijssen, Kirsten L. Larson, Jing Li, Daizhong Liu, Laura A. Lopez, Eric J. Murphy, Lukas Neumann, Jérôme Pety, Francesca Pinna, Miguel Querejeta, Florent Renaud, Toshiki Saito, Sumit K. Sarbadhicary, Amy Sardone, Rowan J. Smith, Sophia K. Stuber, Jiayi Sun, David A. Thilker, Antonio Usero, Bradley C. Whitmore, Thomas G. Williams
Publikováno v:
The Astrophysical Journal Letters, Vol 944, Iss 2, p L22 (2023)
We present a high-resolution view of bubbles within the Phantom Galaxy (NGC 628), a nearby (∼10 Mpc), star-forming (∼2 M _⊙ yr ^−1 ), face-on ( i ∼ 9°) grand-design spiral galaxy. With new data obtained as part of the Physics at High Angul
Externí odkaz:
https://doaj.org/article/552718e6778d4d7a82cabcfce53a38b6
Autor:
Eva Schinnerer, Eric Emsellem, Jonathan D. Henshaw, Daizhong Liu, Sharon E. Meidt, Miguel Querejeta, Florent Renaud, Mattia C. Sormani, Jiayi Sun, Oleg V. Egorov, Kirsten L. Larson, Adam K. Leroy, Erik Rosolowsky, Karin M. Sandstrom, T. G. Williams, Ashley. T. Barnes, F. Bigiel, Mélanie Chevance, Yixian Cao, Rupali Chandar, Daniel A. Dale, Cosima Eibensteiner, Simon C. O. Glover, Kathryn Grasha, Stephen Hannon, Hamid Hassani, Jaeyeon Kim, Ralf S. Klessen, J. M. Diederik Kruijssen, Eric J. Murphy, Justus Neumann, Hsi-An Pan, Jérôme Pety, Toshiki Saito, Sophia K. Stuber, Robin G. Treß, Antonio Usero, Elizabeth J. Watkins, Bradley C. Whitmore, PHANGS
Publikováno v:
The Astrophysical Journal Letters, Vol 944, Iss 2, p L15 (2023)
Large-scale bars can fuel galaxy centers with molecular gas, often leading to the development of dense ringlike structures where intense star formation occurs, forming a very different environment compared to galactic disks. We pair ∼0.″3 (30 pc)
Externí odkaz:
https://doaj.org/article/6ebd9f3476e241b49c997fc8016ca42f
Autor:
Mattia C Sormani, Ashley T Barnes, Jiayi Sun, Sophia K Stuber, Eva Schinnerer, Eric Emsellem, Adam K Leroy, Simon C O Glover, Jonathan D Henshaw, Sharon E Meidt, Justus Neumann, Miguel Querejeta, Thomas G Williams, Frank Bigiel, Cosima Eibensteiner, Francesca Fragkoudi, Rebecca C Levy, Kathryn Grasha, Ralf S Klessen, J M Diederik Kruijssen, Nadine Neumayer, Francesca Pinna, Erik W Rosolowsky, Rowan J Smith, Yu-Hsuan Teng, Robin G Tress, Elizabeth J Watkins
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73d7f4473f09dd4551456f03e7f833d9
Autor:
Janice C. Lee, Karin M. Sandstrom, Adam K. Leroy, David A. Thilker, Eva Schinnerer, Erik Rosolowsky, Kirsten L. Larson, Oleg V. Egorov, Thomas G. Williams, Judy Schmidt, Eric Emsellem, Gagandeep S. Anand, Ashley T. Barnes, Francesco Belfiore, Ivana Bešlić, Frank Bigiel, Guillermo A. Blanc, Alberto D. Bolatto, Médéric Boquien, Jakob den Brok, Yixian Cao, Rupali Chandar, Jérémy Chastenet, Mélanie Chevance, I-Da Chiang, Enrico Congiu, Daniel A. Dale, Sinan Deger, Cosima Eibensteiner, Christopher M. Faesi, Simon C. O. Glover, Kathryn Grasha, Brent Groves, Hamid Hassani, Kiana F. Henny, Jonathan D. Henshaw, Nils Hoyer, Annie Hughes, Sarah Jeffreson, María J. Jiménez-Donaire, Jaeyeon Kim, Hwihyun Kim, Ralf S. Klessen, Eric W. Koch, Kathryn Kreckel, J. M. Diederik Kruijssen, Jing Li, Daizhong Liu, Laura A. Lopez, Daniel Maschmann, Ness Mayker Chen, Sharon E. Meidt, Eric J. Murphy, Justus Neumann, Nadine Neumayer, Hsi-An Pan, Ismael Pessa, Jérôme Pety, Miguel Querejeta, Francesca Pinna, M. Jimena Rodríguez, Toshiki Saito, Patricia Sánchez-Blázquez, Francesco Santoro, Amy Sardone, Rowan J. Smith, Mattia C. Sormani, Fabian Scheuermann, Sophia K. Stuber, Jessica Sutter, Jiayi Sun, Yu-Hsuan Teng, Robin G. Treß, Antonio Usero, Elizabeth J. Watkins, Bradley C. Whitmore, Alessandro Razza
Publikováno v:
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Universidad Nacional de La Plata
instacron:UNLP
The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e2c457b5d160879a96e870a8e70d87d
http://arxiv.org/abs/2212.02667
http://arxiv.org/abs/2212.02667
Autor:
Cara Battersby, Mattia C. Sormani, Paul C. Clark, Rowan J. Smith, Robin G. Tress, Simon C. O. Glover, H Perry Hatchfield, Ralf S. Klessen
Publikováno v:
Sormani, M C, Tress, R G, Glover, S C O, Klessen, R S, Battersby, C D, Clark, P C, Hatchfield, H P & Smith, R J 2020, ' Simulations of the Milky Way’s central molecular zone-II. Star formation ', Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/staa1999
The Milky Way's central molecular zone (CMZ) has emerged in recent years as a unique laboratory for the study of star formation. Here we use the simulations presented in Tress et al. 2020 to investigate star formation in the CMZ. These simulations re
Autor:
Catherine Zucker, Rowan J. Smith, Paul C. Clark, Robin G. Treß, Mattia C. Sormani, Andrés F. Izquierdo, Simon C. O. Glover, Ralf S. Klessen, Ana Duarte Cabral
Publikováno v:
Smith, R, Treß, R G, Sormani, M, Glover, S C O, Klessen, R S, Clark, P C, Izquierdo Cartagena, A F, Cabral, A & Zucker, C 2019, ' The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces ', Monthly Notices of the Royal Astronomical Society, vol. 492, no. 2, pp. 1594-1613 . https://doi.org/10.1093/mnras/stz3328
We introduce a new suite of simulations, "The Cloud Factory", which self-consistently forms molecular cloud complexes at high enough resolution to resolve internal substructure (up to 0.25 Msol in mass) all while including galactic-scale forces. We u
The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
Autor:
Paul C. Clark, Ana Duarte-Cabral, Simon C. O. Glover, Catherine Zucker, Mattia C. Sormani, Robin G. Treß, Andrés F. Izquierdo, Ralf S. Klessen, Rowan J. Smith
Publikováno v:
Izquierdo, A F, Smith, R J, Glover, S C O, Klessen, R S, Treß, R G, Sormani, M C, Clark, P C, Duarte-cabral, A & Zucker, C 2020, ' The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential ', Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/staa3470
Monthly Notices of the Royal Astronomical Society, 500(4), 5268-5296
Monthly Notices of the Royal Astronomical Society, 500(4), 5268-5296
We present a statistical analysis of the gravoturbulent velocity fluctuations in molecular cloud complexes extracted from our "Cloud Factory" galactic-scale ISM simulation suite. For this purpose, we produce non-LTE $^{12}$CO J=1-0 synthetic observat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2026df8112b658db98a46a6551012a4f
https://doi.org/10.1093/mnras/staa3470
https://doi.org/10.1093/mnras/staa3470
Autor:
Mattis Magg, Anna T. P. Schauer, Ralf S. Klessen, Simon C. O. Glover, Robin G. Tress, Ondrej Jaura
Publikováno v:
The Astrophysical Journal. 929:119
The lack of observations of abundance patterns originating in pair-instability supernovae has been a long-standing problem in relation to the first stars. This class of supernovae is expected to have an abundance pattern with a strong odd-even effect