Ultraviolet Perspectives on Diffuse Gas in the Largest Cosmic Structures

Autor: Burchett, J., Butsky, I., Tremmel, M., Bordoloi, R., Bryan, G., Cai, Z., Canning, R., Chen, H., Coil, A., Fielding, D., Fumagalli, M., Johnson, S.D., Khaire, V., Lee, K., Lehner, N., Mandelker, N., O'Meara, J., Muzahid, S., Nelson, D., Oppenheimer, B.D., Postman, M., Peeples, M.S., Quinn, T., Rafelski, M., Ribaudo, J., Rubin, K., Stern, J., Tejos, N., Tonnesen, S., Tripp, T., Wang, Q., Willmer, C.N.A., Zheng, Y.
Přispěvatelé: Burchett, J, Butsky, I, Tremmel, M, Bordoloi, R, Bryan, G, Cai, Z, Canning, R, Chen, H, Coil, A, Fielding, D, Fumagalli, M, Johnson, S, Khaire, V, Lee, K, Lehner, N, Mandelker, N, O'Meara, J, Muzahid, S, Nelson, D, Oppenheimer, B, Postman, M, Peeples, M, Quinn, T, Rafelski, M, Ribaudo, J, Rubin, K, Stern, J, Tejos, N, Tonnesen, S, Tripp, T, Wang, Q, Willmer, C, Zheng, Y
Jazyk: angličtina
Rok vydání: 2019
Předmět:
Zdroj: Bulletin of the American Astronomical Society, 51(3), 534
Popis: The past decade has seen an explosion of discoveries and new insights into the diffuse gas within galaxies, galaxy clusters, and the filaments composing the Cosmic Web. A new decade will bring fresh opportunities to further this progress towards developing a comprehensive view of the composition, thermal state, and physical processes of diffuse gas in the Universe. Ultraviolet (UV) spectroscopy, probing diffuse 10^4-10^6 K gas at high spectral resolution, is uniquely poised to (1) witness environmental galaxy quenching processes in action, such as strangulation and tidal- and ram-pressure stripping, (2) directly account for the baryon content of galaxy clusters in the cold-warm (T
Databáze: OpenAIRE