A Multi-wavelength Study of the Star-forming Core Ahead of HH 80N

Astrophysical Journal

dc.creatorMasque, J.
dc.creatorGaray, G.
dc.date2020-03-11T20:36:30Z
dc.date2022-07-08T17:15:57Z
dc.date2020-03-11T20:36:30Z
dc.date2022-07-08T17:15:57Z
dc.date2011
dc.date.accessioned2023-08-22T03:50:26Z
dc.date.available2023-08-22T03:50:26Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/241000
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8316870
dc.descriptionWe present observations of continuum emission in the mid-infrared to millimeter wavelength range, complemented with ammonia observations, of the dense core ahead of the radio Herbig-Haro (HH) object HH 80N, found in the GGD 27 region. The continuum emissi
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-637X/738/1/43
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleA Multi-wavelength Study of the Star-forming Core Ahead of HH 80N
dc.titleAstrophysical Journal
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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