Results 81 to 90 of about 280,504 (183)
ACES: The Magnetic Field in Large Filaments in the Galactic Center
The Astrophysical JournalThe Galactic center (GC) is an extreme region of the Milky Way that is host to a complex set of thermal and nonthermal structures. In particular, the GC contains high-density gas and dust that is collectively referred to as the Central Molecular Zone ...Dylan M. Paré, Zi-Xuan Feng, Yue Hu, Maya A. Petkova, Jack Sullivan, Robin G. Tress, Cara Battersby, Janik Karoly, Alex Lazarian, Dani Lipman, Xing Pan, Marco Donati, Mattia C. Sormani, John Bally, Ashley T. Barnes, Natalie O. Butterfield, Laura Colzi, Christoph Federrath, Pablo Garcia, Adam Ginsburg, Savannah R. Gramze, Anika Schmiedeke, Christian Henkel, Jonathan D. Henshaw, Paul T. Ho, Pei-Ying Hsieh, Izaskun Jimenez-Serra, Ralf S. Klessen, J. M. Diederik Kruijssen, Steven N. Longmore, Xing Lu, Elisabeth A.C. Mills, Álvaro Sánchez-Monge, Daniel L. Walker, Jennifer Wallace, Qizhou Zhang +35 moredoaj +1 more sourceMultiscale Mass-assembly Scenario in the High-mass Star-forming Filament IRAS 19368+2239 Observed as Part of the INFANT Survey
The Astrophysical JournalA multiscale dynamical mass-assembly scenario, where stars form through multiscale fragmentation and hierarchical gas infall from clouds to filaments, clumps, and cores, has been proposed for high-mass star formation, but the precise observational ...Chengzhi Meng, Hong-Li Liu, Xing Lu, Yu Cheng, R. Galván-Madrid, H. B. Liu, Q. Zhang, S. H. Li, A.E. Guzmán, P. Sanhueza, Kei E. I. Tanaka +10 moredoaj +1 more sourceInterstellar filaments and the statistics of galactic HI
, 2007 This paper presents a statistical explanation of filament formation in the galactic atomic hydrogen. We claim that even in the absence of dynamical factors the Gaussian field corresponding to the measured values of the spectrum of random density should ...A. Lazarian, Lazarian Pogosyan, D. Pogosyan +2 morecore Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations
The Astrophysical JournalWe report 850 μ m continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B -fields In STar forming Regions Observations large program on the James Clerk Maxwell Telescope. These data reveal Jia-Wei Wang, Patrick M. Koch, Seamus D. Clarke, Gary Fuller, Nicolas Peretto, Ya-Wen Tang, Hsi-Wei Yen, Shih-Ping Lai, Nagayoshi Ohashi, Doris Arzoumanian, Doug Johnstone, Ray Furuya, Shu-ichiro Inutsuka, Chang Won Lee, Derek Ward-Thompson, Valentin J. M. Le Gouellec, Hong-Li Liu, Lapo Fanciullo, Jihye Hwang, Kate Pattle, Frédérick Poidevin, Mehrnoosh Tahani, Takashi Onaka, Mark G. Rawlings, Eun Jung Chung, Junhao Liu, A-Ran Lyo, Felix Priestley, Thiem Hoang, Motohide Tamura, David Berry, Pierre Bastien, Tao-Chung Ching, Simon Coudé, Woojin Kwon, Mike Chen, Chakali Eswaraiah, Archana Soam, Tetsuo Hasegawa, Keping Qiu, Tyler L. Bourke, Do-Young Byun, Zhiwei Chen, Huei-Ru Vivien Chen, Wen Ping Chen, Jungyeon Cho, Minho Choi, Yunhee Choi, Youngwoo Choi, Antonio Chrysostomou, Sophia Dai, James Di Francesco, Pham Ngoc Diep, Yasuo Doi, Yan Duan, Hao-Yuan Duan, David Eden, Jason Fiege, Laura M. Fissel, Erica Franzmann, Per Friberg, Rachel Friesen, Tim Gledhill, Sarah Graves, Jane Greaves, Matt Griffin, Qilao Gu, Ilseung Han, Saeko Hayashi, Martin Houde, Tsuyoshi Inoue, Kazunari Iwasaki, Il-Gyo Jeong, Vera Könyves, Ji-hyun Kang, Miju Kang, Janik Karoly, Akimasa Kataoka, Koji Kawabata, Zacariyya Khan, Mi-Ryang Kim, Kee-Tae Kim, Kyoung Hee Kim, Shinyoung Kim, Jongsoo Kim, Hyosung Kim, Gwanjeong Kim, Florian Kirchschlager, Jason Kirk, Masato I. N. Kobayashi, Takayoshi Kusune, Jungmi Kwon, Kevin Lacaille, Chi-Yan Law, Sang-Sung Lee, Hyeseung Lee, Jeong-Eun Lee, Chin-Fei Lee, Dalei Li, Hua-bai Li, Guangxing Li, Di Li, Sheng-Jun Lin, Tie Liu, Sheng-Yuan Liu, Xing Lu, Steve Mairs, Masafumi Matsumura, Brenda Matthews, Gerald Moriarty-Schieven, Tetsuya Nagata, Fumitaka Nakamura, Hiroyuki Nakanishi, Nguyen Bich Ngoc, Geumsook Park, Harriet Parsons, Tae-Soo Pyo, Lei Qian, Ramprasad Rao, Jonathan Rawlings, Brendan Retter, John Richer, Andrew Rigby, Sarah Sadavoy, Hiro Saito, Giorgio Savini, Masumichi Seta, Ekta Sharma, Yoshito Shimajiri, Hiroko Shinnaga, Xindi Tang, Hoang Duc Thuong, Kohji Tomisaka, Le Ngoc Tram, Yusuke Tsukamoto, Serena Viti, Hongchi Wang, Anthony Whitworth, Jintai Wu, Jinjin Xie, Meng-Zhe Yang, Hyunju Yoo, Jinghua Yuan, Hyeong-Sik Yun, Tetsuya Zenko, Chuan-Peng Zhang, Yapeng Zhang, Guoyin Zhang, Jianjun Zhou, Lei Zhu, Ilse de Looze, Philippe André, C. Darren Dowell, Stewart Eyres, Sam Falle, Jean-François Robitaille, Sven van Loo +156 moredoaj +1 more sourceCharacterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArT\'eMiS [PDF]
, 2016 International audienceHerschel observations of nearby molecular clouds suggest that interstellar filaments and prestellar cores represent two fundamental steps in the star formation process.L. Rodriguez, Delisle, C., Hennemann, M., Bontemps, Sylvain, Doumayrou, E., Gallais, P., Palmeirim, P., Schneider, N.,, N. Schneider, Bontemps, S., Dumaye, L., P. Gallais, Dubreuil, D.,, Martignac, J.,, D. Dubreuil, Visticot, F.,, Minier, V.,, Lortholary, M., Doumayrou, E.,, Zavagno, Annie, F. Visticot, Talvard, M.,, Arzoumanian, D., D. Russeil, Peretto, N., Visticot, F., André, Ph.,, Arzoumanian, D.,, Reveret, V., Rodriguez, L.,, K. L. J. Rygl, Motte, F., Roy, A.,, Andre, Ph., H. Roussel, S. Bontemps, Schneider, N., L. Dumaye, V. Minier, Russeil, D., Minier, V., Dubreuil, D., Motte, F.,, P. Palmeirim, Rodriguez, L., T. Hill, Dumaye, L.,, J. Le Pennec, Könyves, V., Roussel, H.,, de Breuck, C.,, Rygl, K. L. J.,, F. Motte, Könyves, V.,, Peretto, N.,, Koenyves, V., M. Lortholary, A. Roy, Revéret, V.,, V. Revéret, Ph. André, Tigé, J.,, Palmeirim, P.,, Hill, T., M. Talvard, J. Tigé, D. Arzoumanian, RYGL, Kazi Lucie Jessica, Le Pennec, Jean-Luc, Roussel, H., Peretto, Nicolas, Shimajiri, Y.,, Rygl, K. L. J., V. Könyves, Y. Shimajiri, A. Zavagno, Roy, A., Hill, T.,, Andre, P. h., Könyves, Vera, Le Pennec, J.,, E. Doumayrou, Le Pennec, J., Zavagno, A., Gallais, P.,, Martignac, J., Delisle, C.,, Shimajiri, Y., M. Hennemann, N. Peretto, Talvard, M., C. De Breuck, C. Delisle, J. Martignac, Lortholary, M.,, Tige, J., De Breuck, C., Russeil, D., +97 morecore +1 more sourceDust in and Around the Heliosphere and Astrospheres. [PDF]
Space Sci Rev, 2022 Sterken VJ, Baalmann LR, Draine BT, Godenko E, Herbst K, Hsu HW, Hunziker S, Izmodenov V, Lallement R, Slavin JD. +9 moreeuropepmc +1 more sourceCluster Formation in a Filamentary Cloud: The Case of the Stellar Cluster NGC 2316
The Astronomical JournalWe present a multiwavelength analysis of the star cluster NGC 2316 and its surroundings. We estimated the physical parameters of the NGC 2316 cluster, including its shape (elongated), size ( R _cluster = 0.4 pc), distance (1.3 ± 0.3 kpc), and minimum ...Saurabh Sharma, Aayushi Verma, Kshitiz Mallick, Lokesh K. Dewangan, Harmeen Kaur, Ram Kesh Yadav, Neelam Panwar, Devendra K. Ojha, Tarak Chand, Mamta Agarwal +9 moredoaj +1 more source
