The implications of the surprising existence of a large, massive CO disk in a distant protocluster

The implications of the surprising existence of a large, massive CO disk in a distant protocluster

It is not yet known if the properties of molecular gas in distant protocluster galaxies are significantly affected by their environment as galaxies are in local clusters. Through a deep, 64 h of effective on-source integration with the Australian Telescope Compact Array (ATCA), we discovered a massi...

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Bibliographic Details
Main Authors: Dannerbauer, H., Lehnert, M.D., Emonts, B., Ziegler, B., Altieri, B., De Breuck, C., Hatch, N., Kodama, T., Koyama, Y., Kurk, J.D., Matiz, T., Miley, G., Narayanan, D., Norris, R.P., Overzier, R., Röttgering, H.J.A., Sargent, M., Seymour, N., Tanaka, M., Valtchanov, I., Wylezalek, D.
Format: Article
Published: EDP Sciences 2017
Subjects:
galaxies: clusters: individual: MRC 1138 / 262 ; galaxies: high-redshift ; galaxies: evolution ; galaxies: ISM ; submillimeter: galaxies ; galaxies: individual: HAE229
Online Access:https://eprints.nottingham.ac.uk/49201/

Internet

https://eprints.nottingham.ac.uk/49201/

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