A fresh view of Henize 2-10 with VLT NAOS-CONICA

Simple item page
dc.contributor.authorCabanac, RA
dc.contributor.authorVanzi, L
dc.contributor.authorSauvage, M
dc.date.accessioned2025-01-21T01:06:44Z
dc.date.available2025-01-21T01:06:44Z
dc.date.issued2005
dc.description.abstractWe present high-resolution observations of Henize 2-10 in K-s (2.2 mu m), L ' (3.8 mu m), and M ' (4.8 mu m) bands. These allow us, for the first time, to track accurately the structures at the heart of the galaxy from the optical to the radio. All radio knots previously observed can now be associated with L '- and K-s-emitting regions. This implies a revision of their physical nature. Instead of highly extinguished ultradense H II regions, we propose that two of the five radio knots are either supernova remnants or normal H II regions, while the remaining three are bona fide ultradense H II regions, although less obscured than previously thought.
dc.fuente.origenWOS
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/96212
dc.identifier.wosidWOS:000231959100017
dc.issue.numero1
dc.language.isoen
dc.pagina.final261
dc.pagina.inicio252
dc.revistaAstrophysical journal
dc.rightsacceso restringido
dc.subjectgalaxies : individual (Henize 2-10)
dc.titleA fresh view of Henize 2-10 with VLT NAOS-CONICA
dc.typeartículo
dc.volumen631
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
Files
Collections
Artículos de revistas