Ultraviolet Perspectives on Diffuse Gas in the Largest Cosmic Structures

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, th...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Hauptverfasser:	Burchett, Joseph N, Nagai, Daisuke, Butsky, Iryna, Tremmel, Michael, Bordoloi, Rongmon, Bryan, Greg, Cai, Zheng, Canning, Rebecca, Chen, Hsiao-Wen, Coil, Alison, Fielding, Drummond, Fumagalli, Michele, Johnson, Sean D, Khaire, Vikram, Lee, Khee-Gan, Lehner, Nicolas, Mandelker, Nir, O'Meara, John, Muzahid, Sowgat, Nelson, Dylan, Oppenheimer, Benjamin D, Postman, Marc, Peeples, Molly S, Quinn, Thomas, Rafelski, Marc, Ribaudo, Joseph, Rubin, Kate, Stern, Jonathan, Tejos, Nicolas, Tonnesen, Stephanie, Tripp, Todd, Wang, Q. Daniel, Willmer, Christopher N. A, Zheng, Yong
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - Astrophysics of Galaxies
Online-Zugang:	Volltext bestellen
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Beschreibung
Zusammenfassung:	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
DOI:	10.48550/arxiv.1903.06201