PAH features in the ISO SWS01 spectra of [WR] planetary nebulae

Author： Szczerba R.  

Publisher： Springer Publishing Company

ISSN： 0004-640X

Source： Astrophysics and Space Science, Vol.275, Iss.1-2, 2001-01, pp. : 113-119

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

ISO-SWS Observations of Planetary Nebulae with [WR] Central Stars

By Szczerba R.  

Astrophysics and Space Science, Vol. 255, Iss. 1-2, 1997-01 ,pp. : 515-521

Springer Publishing Company

Access to resources Recommend Favorite

ISO SWS Spectroscopy of Proto-Planetary Nebulae

By Hrivnak B.J.  

Astrophysics and Space Science, Vol. 255, Iss. 1-2, 1997-01 ,pp. : 477-478

Springer Publishing Company

Access to resources Recommend Favorite

Molecular Features in ISO-SWS Spectra of O-Rich Long-Period Variables

By Kerschbaum F.   Aringer B.   Hron J.   Loidl R.  

Astrophysics and Space Science, Vol. 255, Iss. 1-2, 1997-01 ,pp. : 255-256

Springer Publishing Company

Access to resources Recommend Favorite

ISO-SWS Spectra of Carbon Stars: Molecular Features and a Comparison with Models

By Hron J.  

Astrophysics and Space Science, Vol. 255, Iss. 1-2, 1997-01 ,pp. : 359-360

Springer Publishing Company

Access to resources Recommend Favorite

PAH's and Crystalline Silicates in Planetary Nebulae

By Beintema D.A.  

Astrophysics and Space Science, Vol. 255, Iss. 1-2, 1997-01 ,pp. : 507-512

Springer Publishing Company

Access to resources Recommend Favorite