Zobrazeno 1 - 10
of 118
pro vyhledávání: '"Falgarone, Edith"'
Autor:
Xu, Fengwei, Wang, Ke, Liu, Tie, Eden, David, Liu, Xunchuan, Juvela, Mika, He, Jinhua, Johnstone, Doug, Goldsmith, Paul, Garay, Guido, Wu, Yuefang, Soam, Archana, Traficante, Alessio, Ristorcelli, Isabelle, Falgarone, Edith, Chen, Huei-Ru Vivien, Hirano, Naomi, Doi, Yasuo, Kwon, Woojin, White, Glenn J., Whitworth, Anthony, Sanhueza, Patricio, Rawlings, Mark G., Alina, Dana, Ren, Zhiyuan, Lee, Chang Won, Tatematsu, Ken'ichi, Zhang, Chuan-Peng, Zhou, Jianjun, Lai, Shih-Ping, Ward-Thompson, Derek, Liu, Sheng-Yuan, Gu, Qilao, Chakali, Eswaraiah, Zhu, Lei, Mardones, Diego, Tóth, L. Viktor
High-latitude ($|b|>30^{\circ}$) molecular clouds have virial parameters that exceed 1, but whether these clouds can form stars has not been studied systematically. Using JCMT SCUBA-2 archival data, we surveyed 70 fields that target high-latitude Pla
Externí odkaz:
http://arxiv.org/abs/2401.14658
Publikováno v:
A&A 664, A193 (2022)
Context. An essential facet of turbulence is the space-time intermittency of the cascade of energy that leads to coherent structures of high dissipation. Aims. In this work, we attempt to investigate systematically the physical nature of the intense
Externí odkaz:
http://arxiv.org/abs/2206.03045
Autor:
Luo, Qiuyi, Liu, Tie, Tatematsu, Kenichi, Liu, ShengYuan, Li, Pak Shing, di Francesco, James, Johnstone, Doug, Goldsmith, Paul F., Dutta, Somnath, Hirano, Naomi, Lee, ChinFei, Li, Di, Kim, KeeTae, Lee, Chang Won, Lee, JeongEun, Liu, Xunchuan, Juvela, Mika, He, Jinhua, Qin, ShengLi, Liu, HongLi, Eden, David, Kwon, Woojin, Sahu, Dipen, Li, Shanghuo, Xu, FengWei, Zhang, Siju, Hsu, ShihYing, Bronfman, Leonardo, Sanhueza, Patricio, Pelkonen, VeliMatti, Zhou, Jianwen, Liu, Rong, Gu, Qilao, Wu, Yuefang, Mai, Xiaofeng, Falgarone, Edith, Shen, ZhiQiang
During the transition phase from a prestellar to a protostellar cloud core, one or several protostars can form within a single gas core. The detailed physical processes of this transition, however, still remain unclear. We present 1.3 mm dust continu
Externí odkaz:
http://arxiv.org/abs/2204.06176
Autor:
Lehmann, Andrew, Godard, Benjamin, Forêts, Gillaume Pineau des, Vidal-García, Alba, Falgarone, Edith
Publikováno v:
A&A 658, A165 (2022)
Shocks, modelled over a broad range of parameters, are used to construct a new tool to deduce the mechanical energy and physical conditions from observed atomic or molecular emission lines. We compute magnetised, molecular shock models with velocitie
Externí odkaz:
http://arxiv.org/abs/2111.14089
Autor:
Fissel, Laura, Hull, Charles L. H., Clark, Susan E., Chuss, David T., André, Philippe, Boulanger, François, Dowell, C. Darren, Falgarone, Edith, Hensley, Brandon, Lazarian, A., Novak, Giles, Stephens, Ian, Xu, Siyao
Understanding the physics of how stars form is a highly-prioritized goal of modern Astrophysics, in part because star formation is linked to both galactic dynamics on large scales and to the formation of planets on small scales. It is well-known that
Externí odkaz:
http://arxiv.org/abs/1903.08757
Autor:
Li, Qiong, Cai, Zheng, Prochaska, J. Xavier, Battaia, Fabrizio Arrigoni, Ivison, Rob J., Falgarone, Edith, Cantalupo, Sebastiano, Matuszewski, Matt, Neill, James Don, Wang, Ran, Martin, Chris, Moore, Anna
We present Keck/KCWI integral field spectrograph observations of the complex system surrounding SMM J02399$-$0136 (a lensed $z=2.8$ sub-mm galaxy), including an associated Ly$\rm \alpha$ nebula, a dust-obscured, broad-absorption-line quasar, and neig
Externí odkaz:
http://arxiv.org/abs/1903.03131
Autor:
Godard, Benjamin, Forêts, Guillaume Pineau des, Lesaffre, Pierre, Lehmann, Andrew, Gusdorf, Antoine, Falgarone, Edith
Aims. The goal of the paper is to present a detailed study of the propagation of low velocity (5 to 25 km s-1) stationary molecular shocks in environments illuminated by an external ultraviolet (UV) radiation field. In particular, we intend to show h
Externí odkaz:
http://arxiv.org/abs/1901.04273
Publikováno v:
The Astrophysical Journal, 2019, Volume 871, Number 1
We utilize the multi-wavelength data of M33 to study the origin of turbulence in its interstellar medium. We find that the HI turbulent energy surface density inside 8 kpc is $\sim1-3~\times~10^{46}$ erg pc$^{-2}$, and has no strong dependence on gal
Externí odkaz:
http://arxiv.org/abs/1812.00019
Autor:
Liu, Tie, Li, Pak Shing, Juvela, Mika, Kim, Kee-Tae, Evans II, Neal J., Di Francesco, James, Liu, Sheng-Yuan, Yuan, Jinghua, Tatematsu, Ken'ichi, Zhang, Qizhou, Ward-Thompson, Derek, Fuller, Gary, Goldsmith, Paul F., Koch, P. M., Sanhueza, Patricio, Ristorcelli, I., Kang, Sung-ju, Chen, Huei-Ru, Hirano, N., Wu, Yuefang, Sokolov, Vlas, Lee, Chang Won, White, Glenn J., Wang, Ke, Eden, David, Li, Di, Thompson, Mark, Pattle, Kate M, Soam, Archana, Nasedkin, Evert, Kim, Jongsoo, Kim, Gwanjeong, Lai, Shih-Ping, Park, Geumsook, Qiu, Keping, Zhang, Chuan-Peng, Alina, Dana, Eswaraiah, Chakali, Falgarone, Edith, Fich, Michel, Greaves, Jane, Gu, Q. -L., Kwon, Woojin, Li, Hua-bai, Malinen, Johanna, Montier, Ludovic, Parsons, Harriet, Qin, Sheng-Li, Rawlings, Mark G., Ren, Zhi-Yuan, Tang, Mengyao, Tang, Y. -W., Toth, L. V., Wang, Jiawei, Wouterloot, Jan, Yi, H. -W., Zhang, H. -W.
Publikováno v:
Liu, T., Li, P. S., Juvela M., et al., 2018, ApJ, 859 ,151
Magnetic field is one of the key agents that play a crucial role in shaping molecular clouds and regulating star formation, yet the complete information on the magnetic field is not well constrained due to the limitations in observations. We study th
Externí odkaz:
http://arxiv.org/abs/1803.09457
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