The MURALES survey V. Jet-induced star formation in 3C 277.3 (Coma A)

dc.contributor.authorCapetti, A.
dc.contributor.authorBalmaverde, B.
dc.contributor.authorTadhunter, C.
dc.contributor.authorMarconi, A.
dc.contributor.authorVenturi, G.
dc.contributor.authorChiaberge, M.
dc.contributor.authorBaldi, R. D.
dc.contributor.authorBaum, S.
dc.contributor.authorGilli, R.
dc.contributor.authorGrandi, P.
dc.contributor.authorMeyer, E. T.
dc.contributor.authorMiley, G.
dc.contributor.authorO'Dea, C.
dc.contributor.authorSparks, W.
dc.contributor.authorTorresi, E.
dc.contributor.authorTremblay, G.
dc.date.accessioned2025-01-20T22:00:30Z
dc.date.available2025-01-20T22:00:30Z
dc.date.issued2022
dc.description.abstractWe present observations obtained with the VLT/MUSE optical integral field spectrograph of the radio source 3C 277.3, located at a redshift of 0.085 and associated with the galaxy Coma A. An emission line region fully enshrouds the double-lobed radio source, which is similar to 60 kpc x 90 kpc in size. Based on the emission line ratios, we identified five compact knots in which the gas ionization is powered by young stars located as far as similar to 60 kpc from the host. The emission line filaments surrounding the radio emission are compatible with ionization from fast shocks (with a velocity of 350-500 km s(-1)), but a contribution from star formation occurring at the edges of the radio source is likely. Coma A might be a unique example in the local Universe in which the expanding outflow triggers star formation throughout the whole radio source.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/202141965
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202141965
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/93732
dc.identifier.wosidWOS:000744641300010
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectgalaxies
dc.subjectactive
dc.subjectgalaxies
dc.subjectISM
dc.subjectgalaxies
dc.subjectnuclei
dc.subjectgalaxies
dc.subjectjets
dc.titleThe MURALES survey V. Jet-induced star formation in 3C 277.3 (Coma A)
dc.typeartículo
dc.volumen657
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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