Zobrazeno 1 - 10
of 53 889
pro vyhledávání: '"Gas content"'
Autor:
Wei, Qiang1,2,3,4 (AUTHOR) 1404579796@qq.com, Chen, Song2,3 (AUTHOR) szxychensong@163.com, Yi, Wangfei1,2,3 (AUTHOR), Gui, Herong2,3 (AUTHOR), Jiang, Wei2,3 (AUTHOR), Li, Fengli2,3 (AUTHOR), Li, Shengjie2,3 (AUTHOR)
Publikováno v:
Scientific Reports. 11/16/2024, Vol. 14 Issue 1, p1-24. 24p.
Autor:
Zakharova, D., Vulcani, B., De Lucia, G., Finn, R. A., Rudnick, G., Combes, F., Castignani, G., Fontanot, F., Jablonka, P., Xie, L., Hirschmann, M.
Galaxy evolution depends on the environment in which galaxies are located. The various physical processes (ram-pressure stripping, tidal interactions, etc.) that can affect the gas content in galaxies have different efficiencies in different environm
Externí odkaz:
http://arxiv.org/abs/2408.17367
Aims. To investigate the influence of distance to filaments and dark matter halos on galaxy cold gas content in the empirical model NeutralUniverseMachine (NUM) and the hydrodynamical simulation IllustrisTNG. Methods. We use DisPerSE to identify cosm
Externí odkaz:
http://arxiv.org/abs/2409.08539
Publikováno v:
Scientific Reports, Vol 14, Iss 1, Pp 1-24 (2024)
Abstract The objective of this work is to investigate the implications of geological influence factors on gas content and geochemical characteristics of deep-buried (> 800 m) coalbed methane (CBM) reservoirs. Results show that bituminous coal account
Externí odkaz:
https://doaj.org/article/0839efa026724226945bf4be05aad54d
Publikováno v:
Scientific Reports. 8/13/2024, Vol. 14 Issue 1, p1-12. 12p.
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
Autor:
Galván-Madrid, Roberto, Díaz-González, Daniel J., Motte, Frédérique, Ginsburg, Adam, Cunningham, Nichol, Menten, Karl M., Armante, Mélanie, Bonfand, Mélisse, Braine, Jonathan, Csengeri, Timea, Dell'Ova, Pierre, Louvet, Fabien, Nony, Thomas, Rivera-Soto, Rudy, Sanhueza, Patricio, Stutz, Amelia M., Wyrowski, Friedrich, Álvarez-Gutiérrez, Rodrigo H., Baug, Tapas, Bontemps, Sylvain, Bronfman, Leonardo, Fernández-López, Manuel, Gusdorf, Antoine, Koley, Atanu, Liu, Hong-Li, Salinas, Javiera, Towner, Allison P. M., Whitworth, Anthony P.
We use the H$41\alpha$ recombination line to create templates of the millimeter free-free emission in the ALMA-IMF continuum maps, which allows to separate it from dust emission. This method complements spectral-index information and extrapolation fr
Externí odkaz:
http://arxiv.org/abs/2407.07359
Publikováno v:
Petroleum Science (KeAi Communications Co.). Oct2024, Vol. 21 Issue 5, p3202-3221. 20p.
Autor:
Chung, D. T., Breysse, P. C., Cleary, K. A., Dunne, D. A., Lunde, J. G. S., Padmanabhan, H., Stutzer, N. -O., Tolgay, D., Bond, J. R., Church, S. E., Eriksen, H. K., Gaier, T., Gundersen, J. O., Harper, S. E., Harris, A. I., Hobbs, R., Ihle, H. T., Kim, J., Lamb, J. W., Lawrence, C. R., Murray, N., Pearson, T. J., Philip, L., Readhead, A. C. S., Rennie, T. J., Wehus, I. K., Woody, D. P.
Publikováno v:
A&A 691, A337 (2024)
The Carbon monOxide Mapping Array Project (COMAP) Pathfinder survey continues to demonstrate the feasibility of line-intensity mapping using high-redshift carbon monoxide (CO) line emission traced at cosmological scales. The latest COMAP Pathfinder p
Externí odkaz:
http://arxiv.org/abs/2406.07512
By combining newly obtained deep GBT 21cm observations with optical spectroscopic data, we present an analysis of the gas content of BreakBRD galaxies, a population denoted by their blue star-forming centers and red quenched disks that do not appear
Externí odkaz:
http://arxiv.org/abs/2406.00635