Pulsar observations and small-scale structure in interstellar H I

Details Pulsar observations and small-scale structure in interstellar H I Pulsar observations and small-scale structure in interstellar H I

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.258p..19d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 258, no. 1, Sept. 1, 1992, p. 19P-21P.

Astronomy and Astrophysics

Astronomy

18

Absorption Spectra, H I Regions, Interstellar Matter, Pulsars, Emission Spectra, Radial Velocity

Scientific paper

If small-scale structure is present in H I clouds, then H I absorption profiles toward pulsars with large proper motions should show changes on a time-scale of a few years. We have compared absorption measurements, made with an interval of about four years, toward two pulsars and find a marginal difference in one of them. If confirmed, this could imply structures on the scale of about 1000 AU in H I clouds.

Affiliated with

Also associated with

No associations

Rating

Pulsar observations and small-scale structure in interstellar H I 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 Pulsar observations and small-scale structure in interstellar H I, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pulsar observations and small-scale structure in interstellar H I will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1769687