The nature of G25.5 + 0.2

Details The nature of G25.5 + 0.2 The nature of G25.5 + 0.2

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.248p..11z&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 248, Jan. 15, 1991, p. 11P-13P.

Astronomy and Astrophysics

Astronomy

13

Planetary Nebulae, Radio Sources (Astronomy), Supernova Remnants, Color, H Ii Regions, Infrared Astronomy Satellite

Scientific paper

Recently, an argument has arisen whether the radio source G25.5 + 0.2 is the youngest supernova remnant in the Galaxy, or the most massive planetary nebula known. In this paper it is shown that a classification as planetary nebula is unlikely. A few objects show similarities with G25.5 + 0.2, most of which are classified as H II regions. Although this does not unambiguously resolve the issue of classification, it appears possible that G25.5 + 0.2 belongs to the group of young outflow objects.

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