Positron Annihilation Radiation from the Inner Galaxy

Details Positron Annihilation Radiation from the Inner Galaxy Positron Annihilation Radiation from the Inner Galaxy

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...559..282k&link_type=abstract

The Astrophysical Journal, Volume 559, Issue 1, pp. 282-295.

Astronomy and Astrophysics

Astronomy

57

Galaxy: Center, Gamma Rays: Observations, Ism: General

Scientific paper

The OSSE instrument on the Compton Gamma Ray Observatory (CGRO) was used to measure the one-dimensional latitudinal and longitudinal distributions of positron annihilation radiation (annihilation line and positronium continuum components) along the inner Galactic ridge. Intensity measurements near the Galactic center (differential relative to background fields offset by 9°-12°) show a symmetrical and spatially narrow bulge around the center (effective FWHMs of 4.9d+/-0.7d in Galactic latitude and 6.3d+/-1.5d in longitude) with significant disk contributions to at least 35° in longitude. The latitude width of the Galactic plane emission away from the Galactic center is only weakly constrained in the current analysis. The longitudinal distribution is well fitted by either a model comprising a narrow (~6.3d FWHM ) Gaussian bulge plus ~35° FWHM Gaussian and CO-like disk components, or by a center-truncated R1/4 spheroid plus exponential disk model. For the latter model, the observed narrow latitudinal distribution near the Galactic center suggests that the bulge is ellipsoidal, although the fits are consistent with a spherical bulge as well. The positronium fraction estimate from the Galactic center direction is 0.93+/-0.04. This, combined with the existing narrow line width measurements for the 511 keV annihilation line, suggests that the bulk of the positron annihilation from the Galactic center direction occurs after positronium formation in a warm environment. The inner Galaxy total annihilation radiation flux intensities of ~10.6×10-3 to ~13.7×10-3 cm-2 s-1 implied by the fitted R1/4 ellipsoid plus exponential disk model (narrow and broad disks, respectively) are in agreement with intensities implied by the 511 keV line flux observed by the broad-field SMM instrument. The double-Gaussian plus CO disk model gives similar agreement if a broad (~12° FWHM) disk component is assumed.

Affiliated with

Also associated with

No associations

Rating

Positron Annihilation Radiation from the Inner Galaxy 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 Positron Annihilation Radiation from the Inner Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Positron Annihilation Radiation from the Inner Galaxy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1484692