Sub-A.U. Structure In Galactic HI

Details Sub-A.U. Structure In Galactic HI Sub-A.U. Structure In Galactic HI

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...20111225m&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #112.25; Bulletin of the American Astronomical Society, Vol. 34, p.1283

Astronomy and Astrophysics

Astronomy

Scientific paper

We have observed fluctuations in the neutral hydrogen (HI) absorption measured towards the pulsar PSR B0329+54 using the 100 meter Green Bank radio telescope (GBT). Due to the sensitivity and sky coverage of the GBT, the brightness of PSR B0329+54, and the large proper motion of this pulsar, it is feasible to measure fluctuations in the HI absorption on time scales of less than one day. We report on initial results from these observations which indicate that structures in the cold (< 100 K) HI exist with size scales less than 1 A.U.

Affiliated with

Also associated with

No associations

Rating

Sub-A.U. Structure In Galactic HI 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 Sub-A.U. Structure In Galactic HI, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sub-A.U. Structure In Galactic HI will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1891080