SciELO - Scientific Electronic Library Online

 
vol.41 issue13D simulations of the fragmentation of photoevaporating clumps embedded in a stellar windWWW database of models of accretion disks irradiated by the central star author indexsubject indexsearch form
Home Pagealphabetic serial listing  

Services on Demand

Journal

Article

Indicators

Related links

  • Have no similar articlesSimilars in SciELO

Share


Revista mexicana de astronomía y astrofísica

Print version ISSN 0185-1101

Abstract

RIESGO, H.  and  LOPEZ, J. A.. H2-12, a misidentified planetary nebula in Kepler SNR. Rev. mex. astron. astrofis [online]. 2005, vol.41, n.1, pp.57-60. ISSN 0185-1101.

Narrow-band direct images and long-slit, echelle spectra are presented for H 2-12. This nebula has been classified as a true planetary nebula. However, the data presented here shows that this object is actually part of the brightest knots and filaments located on the western side of Kepler's supernova remnant. Therefore, H 2-12 must be noted as a misclassified planetary nebula.

Keywords : Hydrodynamics; ISM [Individual (H 2-12)]; ISM [Jets and outflows]; ISM [Planetary nebulae]; ISM [Supernova remnants].

        · abstract in Spanish     · text in English

 

Creative Commons License All the contents of this journal, except where otherwise noted, is licensed under a Creative Commons Attribution License