Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Jameson, K E"'
Autor:
Ma, Y. K., McClure-Griffiths, N. M., Clark, S. E., Gibson, S. J., van Loon, J. Th., Soler, J. D., Putman, M. E., Dickey, J. M., Lee, M. -Y., Jameson, K. E., Uscanga, L., Dempsey, J., Dénes, H., Lynn, C., Pingel, N. M.
High-spatial-resolution HI observations have led to the realisation that the nearby (within few hundreds of parsecs) Galactic atomic filamentary structures are aligned with the ambient magnetic field. Enabled by the high quality data from the Austral
Externí odkaz:
http://arxiv.org/abs/2302.04880
Publikováno v:
A&A 672, A153 (2023)
The Small Magellanic Cloud (SMC) is the closest low-metallicity galaxy to the Milky Way where the dynamical state of molecular clouds can be analyzed. We present a CO(2-1) survey at 9 pc resolution obtained with the APEX telescope in an extensive reg
Externí odkaz:
http://arxiv.org/abs/2211.07792
Autor:
Wong, Tony, Oudshoorn, Luuk, Sofovich, Eliyahu, Green, Alex, Shah, Charmi, Indebetouw, Rémy, Meixner, Margaret, Hacar, Alvaro, Nayak, Omnarayani, Tokuda, Kazuki, Bolatto, Alberto D., Chevance, Mélanie, De Marchi, Guido, Fukui, Yasuo, Hirschauer, Alec S., Jameson, K. E., Kalari, Venu, Lebouteiller, Vianney, Looney, Leslie W., Madden, Suzanne C., Onishi, Toshikazu, Roman-Duval, Julia, Rubio, Mónica, Tielens, A. G. G. M.
Publikováno v:
ApJ, 932, 47 (2022)
We present results of a wide-field (approximately 60 x 90 pc) ALMA mosaic of CO(2-1) and $^{13}$CO(2-1) emission from the molecular cloud associated with the 30 Doradus star-forming region. Three main emission complexes, including two forming a bowti
Externí odkaz:
http://arxiv.org/abs/2206.06528
Autor:
Pingel, N. M., Dempsey, J., McClure-Griffiths, N. M., Dickey, J. M., Jameson, K. E., Arce, H., Anglada, G., Bland-Hawthorn, J., Breen, S. L., Buckland-Willis, F., Clark, S. E., Dawson, J. R., Dénes, H., Di Teodoro, E. M., For, B. -Q., Foster, Tyler J., Gómez, J. F., Imai, H., Joncas, G., Kim, C. -G., Lee, M. -Y., Lynn, C., Leahy, D., Ma, Y. K., Marchal, A., McConnell, D., Miville-Deschênes, M. -A., Moss, V. A., Murray, C. E., Nidever, D., Peek, J., Stanimirović, S., Staveley-Smith, L., Tepper-Garcia, T., Tremblay, C. D., Uscanga, L., van Loon, J. Th., Vázquez-Semadeni, E., Allison, J. R., Anderson, C. S., Ball, Lewis, Bell, M., Bock, D. C. -J., Bunton, J., Cooray, F. R., Cornwell, T., Koribalski, B. S., Gupta, N., Hayman, D. B., Harvey-Smith, L., Lee-Waddell, K., Ng, A., Phillips, C. J., Voronkov, M., Westmeier, T., Whiting, M. T.
We present the most sensitive and detailed view of the neutral hydrogen (HI) emission associated with the Small Magellanic Cloud (SMC), through the combination of data from the Australian Square Kilometre Array Pathfinder (ASKAP) and Parkes (Murriyan
Externí odkaz:
http://arxiv.org/abs/2111.05339
Autor:
Clemens, Dan P., Cashman, L. R., Cerny, C., El-Batal, A. M., Jameson, K. E., Marchwinski, R., Montgomery, J., Pavel, M., Pinnick, A., Taylor, B. W.
The Galactic Plane Infrared Polarization Survey (GPIPS) seeks to characterize the magnetic field in the dusty Galactic disk using near-infrared stellar polarimetry. All GPIPS observations were completed using the 1.83 m Perkins telescope and Mimir in
Externí odkaz:
http://arxiv.org/abs/2006.15203
Autor:
Di Teodoro, Enrico M., McClure-Griffiths, N. M., De Breuck, C., Armillotta, L., Pingel, N. M., Jameson, K. E., Dickey, J. M., Rubio, M., Stanimirovic, S., Staveley-Smith, L.
We report the first evidence of molecular gas in two atomic hydrogen (HI) clouds associated with gas outflowing from the Small Magellanic Cloud (SMC). We used the Atacama Pathfinder Experiment (APEX) to detect and spatially resolve individual clumps
Externí odkaz:
http://arxiv.org/abs/1910.10718
Autor:
Di Teodoro, E. M., McClure-Griffiths, N. M., Jameson, K. E., Denes, H., Dickey, John M., Stanimirovic, S., Staveley-Smith, L., Anderson, C., Bunton, J. D., Chippendale, A., Lee-Waddell, K., MacLeod, A., Voronkov, M. A
We use new high-resolution HI data from the Australian Square Kilometre Array Pathfinder (ASKAP) to investigate the dynamics of the Small Magellanic Cloud (SMC). We model the HI gas component as a rotating disc of non-negligible angular size, moving
Externí odkaz:
http://arxiv.org/abs/1811.09627
Autor:
Oey, M. S., Lopez-Hernandez, J., Kellar, J. A., Pellegrini, E. W., Gordon, K. D., Jameson, K. E., Li, A., Madden, S. C., Meixner, M., Roman-Duval, J., Bot, C., Rubio, M., Tielens, A. G. G. M.
We use the Spitzer SAGE survey of the Magellanic Clouds to evaluate the relationship between the 8-mic PAH emission, 24-mic hot dust emission, and HII region radiative transfer. We confirm that in the higher-metallicity Large Magellanic Cloud, PAH de
Externí odkaz:
http://arxiv.org/abs/1706.04673
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Akademický článek
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