SciELO - Scientific Electronic Library Online

 
vol.42 número2Emission line ratios from variable velocity jet modelsThe composite form of the supernova remnant 3C 400.2: two interacting supernova remnants or a single supernova remnant with a blow-out? 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

PHILLIPS, J. P.. The problem with reddening distances to planetary nebulae. Rev. mex. astron. astrofis [online]. 2006, vol.42, n.2, pp.229-239. ISSN 0185-1101.

It is noted that the vast majority of Galactic PNe are located outside of the interstellar reddening layer, to the extent that local gradients in EB-V are low to undetectable. This is likely to invalidate certain previous estimates of their reddening distances DRED. It also means that larger scale analyses, such as those of Pottasch (1984) and Acker (1973), lead to values of DRED which are significantly too small. A similar critique applies to analyses based on measures of Na D-line absorption, and it seems likely that most of the distances of Napiwotzki & Schönberner (1995) are similarly in error.

Palabras llave : ISM [JETS AND OUTFLOWS]; PLANETARY NEBULAE [GENERAL].

        · 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