Zobrazeno 1 - 10
of 16 115
pro vyhledávání: '"Ellison P"'
Publikováno v:
Journal of Healthcare Leadership, Vol Volume 13, Pp 199-207 (2021)
Matthew A Crain,1 Amy L Bush,2 Heather Hayanga,3 Annelee Boyle,4 Merv Unger,3 Matthew Ellison,3 Pavithra Ellison3 1West Virginia University School of Medicine, Morgantown, WV, USA; 2West Virginia University Medicine Children’s Hospital, Morgantown,
Externí odkaz:
https://doaj.org/article/857cafd93a3f4aa3bac4dc833170adff
Autor:
Ellison, Sara L., Ferreira, Leonardo, Wild, Vivienne, Wilkinson, Scott, Rowlands, Kate, Patton, David R.
(Abridged) Mechanisms for quenching star formation in galaxies remain hotly debated, with galaxy mergers an oft-proposed pathway. In Ellison et al. (2022) we tested this scenario by quantifying the fraction of recently and rapidly quenched post-starb
Externí odkaz:
http://arxiv.org/abs/2410.06357
Autor:
Ferreira, Leonardo, Ellison, Sara L., Patton, David R., Byrne-Mamahit, Shoshannah, Wilkinson, Scott, Bickley, Robert, Conselice, Christopher J., Bottrell, Connor
Galaxy mergers can enhance star formation rates throughout the merger sequence, with this effect peaking around the time of coalescence. However, owing to a lack of information about their time of coalescence, post-mergers could only previously be st
Externí odkaz:
http://arxiv.org/abs/2410.06356
Autor:
Bickley, Robert W., Wilkinson, Scott, Ferreira, Leonardo, Ellison, Sara L., Bottrell, Connor, Jyoti, Debarpita
Studies have shown that the morphologies of galaxies are substantially transformed following coalescence after a merger, but post-mergers are notoriously difficult to identify, especially in imaging that is shallow or low-resolution. We train convolu
Externí odkaz:
http://arxiv.org/abs/2409.17081
Galaxy interactions can trigger drastic changes in the resolved star-forming properties of their constituents, but it remains unclear as to whether those changes are discernible from secular starburst triggers. In this Letter we investigate whether o
Externí odkaz:
http://arxiv.org/abs/2409.15274
Autor:
Wild, Vivienne, Asari, Natalia Vale, Rowlands, Kate, Ellison, Sara L., Leung, Ho-Hin, Tremonti, Christy
In galaxies with significant ongoing star formation there is an impressively tight correlation between total infrared luminosity (L$_{TIR}$) and H$\alpha$ luminosity (L$_{H\alpha}$), when H$\alpha$ is properly corrected for stellar absorption and dus
Externí odkaz:
http://arxiv.org/abs/2409.08672
Autor:
Sargent, Mark T., Ellison, S. L., Mendel, J. T., Saintonge, A., Molnár, D. Cs., Scudder, J. M., Violino, G.
Exploiting IRAM 30 m CO spectroscopy, we find that SDSS post-merger galaxies display gas fractions and depletion times enhanced by 25-50%, a mildly higher CO excitation, and standard molecular-to-atomic gas ratios, compared to non-interacting galaxie
Externí odkaz:
http://arxiv.org/abs/2409.06572
Reconstructing transmission networks is essential for identifying key factors like superspreaders and high-risk locations, which are critical for developing effective pandemic prevention strategies. In this study, we developed a Bayesian framework th
Externí odkaz:
http://arxiv.org/abs/2409.05245
Autor:
Ellison, C. Leland, Garcia, Vincent, Gomez, Matthew, Grim, Gary P., Hammer, Jim H., Jennings, Christopher A., Knapp, Patrick, LeChien, Keith R., Meezan, Nathan, Peterson, Robert, Reyes, Adam, Steiner, Adam, Stygar, William A., Tzeferacos, Petros, Welch, Dale, Zylstra, Alex
Fusion is a potentially transformational energy technology, which promises limitless clean energy. Yet, it requires continued scientific and technological development to realize its potential. The conditions necessary for fusion energy gain in terms
Externí odkaz:
http://arxiv.org/abs/2408.15206
Autor:
Yoon, Hyein, Sadler, Elaine M., Mahony, Elizabeth K., Aditya, J. N. H. S., Allison, James R., Glowacki, Marcin, Kerrison, Emily F., Moss, Vanessa A., Su, Renzhi, Weng, Simon, Whiting, Matthew, Wong, O. Ivy, Callingham, Joseph R., Curran, Stephen J., Darling, Jeremy, Edge, Alastair C., Ellison, Sara L., Emig, Kimberly L., Garratt-Smithson, Lilian, German, Gordon, Grasha, Kathryn, Koribalski, Baerbel S., Morganti, Raffaella, Oosterloo, Tom, Péroux, Céline, Pettini, Max, Pimbblet, Kevin A., Zheng, Zheng, Zwaan, Martin, Ball, Lewis, Bock, Douglas C. -J., Brodrick, David, Bunton, John D., Cooray, F. R., Edwards, Philip G., Hayman, Douglas B., Hotan, Aidan W., Lee-Waddell, K., McClure-Griffiths, N. M., Ng, A., Phillips, Chris J., Raja, Wasim, Voronkov, Maxim A., Westmeier, Tobias
The First Large Absorption Survey in HI (FLASH) is a large-area radio survey for neutral hydrogen in the redshift range 0.4
Externí odkaz:
http://arxiv.org/abs/2408.06626