OH 1720 MHz Masers in the Galactic Center: Sagittarius A East and the Circumnuclear Disk

Details OH 1720 MHz Masers in the Galactic Center: Sagittarius A East and the Circumnuclear Disk OH 1720 MHz Masers in the Galactic Center: Sagittarius A East and the Circumnuclear Disk

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..54...77p&link_type=abstract

"Journal of Physics: Conference Series, Volume 54, Proceedings of "The Universe Under the Microscope - Astrophysics at High Angu

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

We present new and archival Very Large Array (VLA) radio interferometry observations of the 1720 MHz OH masers in the Galactic Center (GC). Most 1720 MHz OH masers arise in regions where the supernova remnant Sgr A East is interacting with the interstellar medium. However, here we also present some previously detected positive velocity masers together with some newly detected negative velocity masers. In combination, those masers appear to bracket Sgr A* in position and velocity. The location and velocities of those masers are consistent with their being in the circumnuclear disk (CND).

Affiliated with

Also associated with

No associations

Rating

OH 1720 MHz Masers in the Galactic Center: Sagittarius A East and the Circumnuclear Disk 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 OH 1720 MHz Masers in the Galactic Center: Sagittarius A East and the Circumnuclear Disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and OH 1720 MHz Masers in the Galactic Center: Sagittarius A East and the Circumnuclear Disk will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1547976