The structure of the emission nebula M 1-78 at 15.4 GHz

Details The structure of the emission nebula M 1-78 at 15.4 GHz The structure of the emission nebula M 1-78 at 15.4 GHz

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.182..657s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 182, Mar. 1978, p. 657-660. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

4

Microwave Emission, Planetary Nebulae, Radio Sources (Astronomy), Astronomical Catalogs, Astronomical Maps, Carbon Monoxide, H Ii Regions, Molecular Spectra

Scientific paper

It is not known whether M1-78 is a planetary nebula or a young H II
region. In an attempt to settle this issue, it has been observed at a
frequency of 15.4 GHz with an angular resolution 0.65 x 0.83 arcsec and
the optical position of the nebula has been remeasured. It is concluded
that the evidence is equivocal and the nature of M1-78 remains in doubt.

Affiliated with

Also associated with

No associations

Rating

The structure of the emission nebula M 1-78 at 15.4 GHz does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The structure of the emission nebula M 1-78 at 15.4 GHz, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The structure of the emission nebula M 1-78 at 15.4 GHz will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1082704