SciELO - Scientific Electronic Library Online

 
vol.49 número2Time Variation of the O/H Radial Gradient in the Galactic Disk Based on Planetary NebulaeAtomic Interpretation of the 13 keV Emission Feature in Three AXPs: 4U 0142+61, XTE J1810-197 and 1E 1048.1-5937 índice de autoresíndice de materiabúsqueda de artículos
Home Pagelista alfabética de revistas  

Servicios Personalizados

Revista

Articulo

Indicadores

Links relacionados

  • No hay artículos similaresSimilares en SciELO

Compartir


Revista mexicana de astronomía y astrofísica

versión impresa ISSN 0185-1101

Resumen

DZIB, Sergio A.; RODRIGUEZ, Luis F.; ARAUDO, Anabelia T.  y  LOINARD, Laurent. Radio Sources Embedded in the Dense Core B59, the "Mouthpiece" of the Pipe Nebula. Rev. mex. astron. astrofis [online]. 2013, vol.49, n.2, pp.345-349. ISSN 0185-1101.

We present Very Large Array continuum observations made at 8.3 GHz toward the dense core B59, in the Pipe Nebula. We detect six compact sources, of which five are associated with the five most luminous sources at 70 μm in the region, while the remaining one is probably a background source. We propose that the radio emission is free-free from the ionized outflows present in these protostars. We discuss the kinematical impact of these winds in the cloud. We also propose that these winds are optically thick in radio but optically thin in X-rays, and that this feature can explain why X-rays from the magnetosphere are detected in three of them, while the radio emission is probably dominated by the free-free emission from the external layers of the wind.

Palabras llave : ISM [individual objects (B59)]; radio continuum [stars]; stars [premain sequence].

        · resumen en Español     · texto en Inglés

 

Creative Commons License Todo el contenido de esta revista, excepto dónde está identificado, está bajo una Licencia Creative Commons