Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Jacob L. Ward"'
Autor:
Marta Sewiło, Martin Cordiner, Steven B. Charnley, Joana M. Oliveira, Emmanuel Garcia-Berrios, Peter Schilke, Jacob L. Ward, Jennifer Wiseman, Remy Indebetouw, Kazuki Tokuda, Jacco Th. van Loon, Álvaro Sánchez-Monge, Veronica Allen, C.-H. Rosie Chen, Roya Hamedani Golshan, Agata Karska, Lars E. Kristensen, Stan E. Kurtz, Thomas Möller, Toshikazu Onishi, Sarolta Zahorecz
Publikováno v:
Astrophysical Journal, 931(2):102. IOP PUBLISHING LTD
Sewilo, M, Cordiner, M, Charnley, S B, Oliveira, J M, Garcia-Berrios, E, Schilke, P, Ward, J L, Wiseman, J, Indebetouw, R, Tokuda, K, van Loon, J T, Sanchez-Monge, A, Allen, V, Chen, C-H R, Hamedani Golshan, R, Karska, A, Kristensen, L E, Kurtz, S E, Moeller, T, Onishi, T & Zahorecz, S 2022, ' ALMA Observations of Molecular Complexity in the Large Magellanic Cloud : The N 105 Star-forming Region ', Astrophysical Journal, vol. 931, no. 2, 102 . https://doi.org/10.3847/1538-4357/ac4e8f
Sewilo, M, Cordiner, M, Charnley, S B, Oliveira, J M, Garcia-Berrios, E, Schilke, P, Ward, J L, Wiseman, J, Indebetouw, R, Tokuda, K, van Loon, J T, Sanchez-Monge, A, Allen, V, Chen, C-H R, Hamedani Golshan, R, Karska, A, Kristensen, L E, Kurtz, S E, Moeller, T, Onishi, T & Zahorecz, S 2022, ' ALMA Observations of Molecular Complexity in the Large Magellanic Cloud : The N 105 Star-forming Region ', Astrophysical Journal, vol. 931, no. 2, 102 . https://doi.org/10.3847/1538-4357/ac4e8f
The Large Magellanic Cloud (LMC) is the nearest laboratory for detailed studies on the formation and survival of complex organic molecules (COMs), including biologically important ones, in low-metallicity environments--typical for earlier cosmologica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5ef7c828b1ccc81c3e164c1e21dee8f
http://arxiv.org/abs/2201.09945
http://arxiv.org/abs/2201.09945
The time-scales associated with various stages of the star formation process represent major unknowns in our understanding of galactic evolution, as well as of star and planet formation. This is the second paper in a series aiming to establish a mult
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4aa75ce6dbcbcbe1c29b121422eb93d4
Autor:
Javier Ballesteros-Paredes, Mark Gieles, Ralf S. Klessen, Stella S. R. Offner, Martin Krause, Jacob L. Ward, Corinne Charbonnel, Enrique Vázquez-Semadeni, J. M. Diederik Kruijssen, Hans Zinnecker, Philipp Girichidis
Publikováno v:
Space Science Reviews
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
arXiv:2005.00801v2
Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is transformed to turbulence with stars forming from cores fed by filaments. In the most compact regions, stellar feedback is least effecti
Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is transformed to turbulence with stars forming from cores fed by filaments. In the most compact regions, stellar feedback is least effecti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e82f007d5f3121d73dbc3a686952b49c
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Historically, it has often been asserted that most stars form in compact clusters. In this scenario, present-day gravitationally-unbound OB associations are the result of the expansion of initially gravitationally-bound star clusters. However, this p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::990e624826d77bf80d3e4789a891586f
http://arxiv.org/abs/1910.06974
http://arxiv.org/abs/1910.06974
Autor:
Jacob L. Ward, Steven B. Charnley, Roya Hamedani Golshan, Remy Indebetouw, M. Sewilo, Sarolta Zahorecz, C.-H. Rosie Chen, Vianney Taquet, Akiko Kawamura, Yasuo Fukui, Jennifer Wiseman, Peter Schilke, Eva Wirström, Jacco Th. van Loon, Joana M. Oliveira, Toshikazu Onishi, Takashi Shimonishi
Publikováno v:
ACS Earth and Space Chemistry
The Large and Small Magellanic Clouds (LMC and SMC), gas-rich dwarf companions of the Milky Way, are the nearest laboratories for detailed studies on the formation and survival of complex organic molecules (COMs) under metal poor conditions. To date,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::642c69c3283895db29e8441a5ffe5dea
Publikováno v:
Monthly Notices of the Royal Astronomical Society
It is often stated that star clusters are the fundamental units of star formation and that most (if not all) stars form in dense stellar clusters. In this monolithic formation scenario, low density OB associations are formed from the expansion of gra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d42ebd66094a93c21d3f682229c31604
http://arxiv.org/abs/1801.03938
http://arxiv.org/abs/1801.03938
Autor:
Jacco Th. van Loon, Jennifer Wiseman, Peter Schilke, Yasuo Fukui, Joana M. Oliveira, C.-H. Rosie Chen, Jacob L. Ward, Margaret Meixner, Sarolta Zahorecz, Toshikazu Onishi, Remy Indebetouw, Steven B. Charnley, Akiko Kawamura, Marta Sewilo
Publikováno v:
The Astrophysical Journal. 853:L19
We report the first extragalactic detection of the complex organic molecules (COMs) dimethyl ether (CH$_3$OCH$_3$) and methyl formate (CH$_3$OCHO) with the Atacama Large Millimeter/submillimeter Array (ALMA). These COMs together with their parent spe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98be36fe393af76ef287c3fcc4f406e7
https://doi.org/10.3847/2041-8213/aaa079
https://doi.org/10.3847/2041-8213/aaa079
Publikováno v:
Proceedings of the International Astronomical Union. 11
At distances of ~50 kpc and ~60 kpc for the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) respectively the Magellanic Clouds present us with a unique opportunity to study star formation in environments outside our own galaxy. Through
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::827c8d5c4108253eb41aa7ade2a0fdd2
https://doi.org/10.1017/s1743921316008449
https://doi.org/10.1017/s1743921316008449
Autor:
Brent Groves, Kathryn Kreckel, Daniel A. Dale, Antonio Usero, Kathryn Grasha, Jiayi Sun, Cinthya N. Herrera, Guillermo A. Blanc, Christopher M Faesi, Ralf S. Klessen, Frank Bigiel, J. M. Diederik Kruijssen, Yixian Cao, Eva Schinnerer, Jacob L. Ward, Simon C. O. Glover, Thomas G. Williams, Miguel Querejeta, Karin Sandstrom, Janice C. Lee, Mélanie Chevance, Ashley T. Barnes, Jérôme Pety, Andreas Schruba, Jaeyeon Kim, Adam K. Leroy
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 504 (1), pp.487-509. ⟨10.1093/mnras/stab878⟩
MNRAS
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 504 (1), pp.487-509. ⟨10.1093/mnras/stab878⟩
MNRAS
Feedback from massive stars plays a key role in molecular cloud evolution. After the onset of star formation, the young stellar population is exposed by photoionization, winds, supernovae, and radiation pressure from massive stars. Recent observation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a7c218544ee6928c5ca83d5c61f9d87
Autor:
Alexander P. S. Hygate, Jacob L. Ward, J. M. Diederik Kruijssen, Steven N. Longmore, Mélanie Chevance, Andreas Schruba
The time-scales associated with the various stages of the star formation process remain poorly constrained. This includes the earliest phases of star formation, during which molecular clouds condense out of the atomic interstellar medium. We present
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1ada89f22ccb73252031e3224cb73005
https://researchonline.ljmu.ac.uk/id/eprint/13327/8/staa1977.pdf
https://researchonline.ljmu.ac.uk/id/eprint/13327/8/staa1977.pdf