Upper limits to interstellar PO

Details Upper limits to interstellar PO Upper limits to interstellar PO

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...312..358m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 312, Jan. 1, 1987, p. 358-362.

Astronomy and Astrophysics

Astrophysics

16

Interstellar Matter, Microwave Spectra, Molecular Clouds, Molecular Ions, Phosphorus Oxides, Abundance, Cosmochemistry, Reaction Kinetics

Scientific paper

Laboratory work has established that PO is likely to be the most abundant molecule containing phosphorus in dense interstellar clouds. Using recently measured microwave frequencies, the authors have searched for the J = 5/2→3/2 transition of PO at 109 GHz in four galactic sources. The limit in DR 21(OH), in particular, suggests that phosphorus may be severely depleted in dense molecular clouds.

Affiliated with

Also associated with

No associations

Rating

Upper limits to interstellar PO 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 Upper limits to interstellar PO, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Upper limits to interstellar PO will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1622254