0484378 - ASÚ 2018 RIV US eng J - Článek v odborném periodiku
Jáchym, Pavel - Sun, M. - Kenney, J.D.P. - Cortese, L. - Combes, F. - Yagi, M. - Yoshida, M. - Palouš, Jan - Roediger, E.
Molecular Gas Dominated 50 kpc Ram Pressure Stripped Tail of the Coma Galaxy D100.
Astrophysical Journal. Roč. 839, č. 2 (2017), 114/1-114/15. ISSN 0004-637X. E-ISSN 1538-4357
Grant CEP: GA MŠMT LG14013; GA ČR GA15-06012S; GA MŠMT(CZ) LM2015067
Institucionální podpora: RVO:67985815
Klíčová slova: galaxies * clusters * evolution
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.551, rok: 2017 ; AIS: 1.755, rok: 2017
DOI: https://doi.org/10.3847/1538-4357/aa6af5

We have discovered large amounts of molecular gas, as traced by CO emission, in the ram pressure stripped gas tail of the Coma cluster galaxy D100 (GMP 2910), out to large distances of about 50 kpc. D100 has a 60 kpc long, strikingly narrow tail, which is bright in X-rays and Ha.
Trvalý link: http://hdl.handle.net/11104/0279546