Zobrazeno 1 - 10
of 127
pro vyhledávání: '"G, Knee"'
Autor:
Miranda Caputo, Archana Soam, B-G Andersson, Remy Dennis, Ed Chambers, Rolf Güsten, Lewis B. G. Knee, Jürgen Stutzki
Publikováno v:
The Astrophysical Journal, Vol 950, Iss 2, p 140 (2023)
We used high-resolution [C ii ] 158 μ m mapping of two nebulae IC 59 and IC 63 from SOFIA/upGREAT in conjunction with ancillary data of the gas, dust, and polarization to probe the kinematics, structure, and magnetic properties of their photodissoci
Externí odkaz:
https://doaj.org/article/96bbe146908f4bed8951606517cc8ab4
Autor:
Lars Bonne, B-G Andersson, Robert Minchin, Archana Soam, Joshua Yaldaei, Kristin Kulas, Janik Karoly, Lewis B. G. Knee, Siddharth Kumar, Nirupam Roy
Publikováno v:
The Astronomical Journal, Vol 165, Iss 6, p 243 (2023)
Photodissociation regions (PDRs), where the (far-)ultraviolet light from hot young stars interact with the gas in surrounding molecular clouds, provide laboratories for understanding the nature and role of feedback by star formation on the interstell
Externí odkaz:
https://doaj.org/article/c1328b907c674001a0381b9ea165a560
Publikováno v:
IEEE Transactions on Microwave Theory and Techniques. :1-16
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::760ce935881cfe085139c12e4b5b6999
https://doi.org/10.1109/tmtt.2023.3267544
https://doi.org/10.1109/tmtt.2023.3267544
Autor:
Lars Bonne, B-G Andersson, Robert Minchin, Archana Soam, Joshua Yaldaei, Kristin Kulas, Janik Karoly, Lewis B. G. Knee, Siddharth Kumar, Nirupam Roy
Photodissociation regions (PDRs), where the (far-)ultraviolet light from hot young stars interact with the gas in surrounding molecular clouds, provide laboratories for understanding the nature and role of feedback by star formation on the interstell
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2bd2db4df7b2eb7e4ab19b92aeb83c7
Publikováno v:
Journal of Astronomical Telescopes, Instruments, and Systems. 8
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::71648d57b22f213c57fd69ad1f60a47a
https://doi.org/10.1117/1.jatis.8.3.036004
https://doi.org/10.1117/1.jatis.8.3.036004
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cc9cddca6ec760f56771bf1e62c63f55
https://doi.org/10.1117/12.2629137
https://doi.org/10.1117/12.2629137
Autor:
Sara Salem Hesari, Doug W. Henke, Vladimir Reshetov, Bruce Veidt, Alireza Seyfollahi, Nianhua Jiang, Lewis B. G. Knee
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4a1eb771f649a0ed2578d4a1e9f50f2c
https://doi.org/10.1117/12.2627870
https://doi.org/10.1117/12.2627870
Autor:
Doug W. Henke, Nianhua Jiang, Sara Salem Hesari, Alireza Seyfollahi, Bruce Veidt, Lewis B. G. Knee
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::53973181ab85c102cc1064e78224638c
https://doi.org/10.1117/12.2630537
https://doi.org/10.1117/12.2630537
Autor:
M. Tahani, J. Glover, W. Lupypciw, J. L. West, R. Kothes, R. Plume, S. Inutsuka, M.-Y. Lee, I. A. Grenier, L. B. G. Knee, J. C. Brown, Y. Doi, T. Robishaw, M. Haverkorn
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 660, ⟨10.1051/0004-6361/202243322⟩
Astronomy & Astrophysics, 660, pp. 1-9
Astronomy & Astrophysics, 660, 1-9
Astronomy and Astrophysics-A&A, 2022, 660, ⟨10.1051/0004-6361/202243322⟩
Astronomy & Astrophysics, 660, pp. 1-9
Astronomy & Astrophysics, 660, 1-9
Magnetic fields permeate the interstellar medium and are important in the star formation process. Determining the 3D magnetic fields of molecular clouds will allow us to better understand their role in the evolution of these clouds and formation of s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c415955e5e93dc25f60585080dd88b1
https://doi.org/10.1051/0004-6361/202243322
https://doi.org/10.1051/0004-6361/202243322
Autor:
M. Tahani, W. Lupypciw, J. Glover, R. Plume, J. L. West, R. Kothes, S. Inutsuka, M.-Y. Lee, T. Robishaw, L. B. G. Knee, J. C. Brown, Y. Doi, I. A. Grenier, M. Haverkorn
Publikováno v:
Astronomy & Astrophysics, 660, 1-13
Astronomy & Astrophysics, 660, pp. 1-13
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 660, ⟨10.1051/0004-6361/202141170⟩
Astronomy & Astrophysics, 660, pp. 1-13
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 660, ⟨10.1051/0004-6361/202141170⟩
Despite recent observational and theoretical advances in mapping the magnetic fields associated with molecular clouds, their three-dimensional (3D) morphology remains unresolved. Multi-wavelength and multi-scale observations will allow us to paint a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20b3b7d13b54bc3e1e8a28008d428ca7
http://hdl.handle.net/2066/249183
http://hdl.handle.net/2066/249183