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The molecular gas content in a protocluster at z = 17: Star..:
D'Amato, Q.
;
Prandoni, I.
;
Gilli, R.
...
Proceedings of the International Astronomical Union. 15 (2019) S352 - p. 168-170 , 2019
Link:
https://doi.org/10.1017/s1743921319009475
RT Journal T1 <Title>The molecular gas content in a protocluster at z = 17: Star formation and AGN feedback</Title> UL https://suche.suub.uni-bremen.de/peid=cr-10.1017_s1743921319009475&Exemplar=1&LAN=DE A1 D'Amato, Q. A1 Prandoni, I. A1 Gilli, R. A1 Massardi, M. A1 Liuzzo, E. A1 Mignoli, M. A1 Vignali, C. A1 Peca, A. A1 Nanni, R. PB Cambridge University Press (CUP) YR 2019 SN 1743-9213 SN 1743-9221 JF Proceedings of the International Astronomical Union VO 15 IS S352 SP 168 OP 170 LK http://dx.doi.org/https://doi.org/10.1017/s1743921319009475 DO https://doi.org/10.1017/s1743921319009475 SF ELIB - SuUB Bremen
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