Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2011-06-28
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
9 pages, 4 figures; accepted to the Astrophysical Journal
Scientific paper
Most pulsars observed by the Fermi LAT have gamma-ray luminosities scaling with spindown power Edot as L_gamma (Edot x 10^33 erg/s)^{1/2}. However, there exist one detection and several upper limits an order of magnitude or more fainter than this trend. We describe these `sub-luminous' gamma-ray pulsars, and discuss the case for this being an orientation effect. Of the 12 known young radio pulsars with Edot>10^34 erg/s and d<2kpc several are substantially sub-luminous. The limited available geometrical constraints favor aligned geometries for these pulsars, although no one case for alignment is compelling. In this scenario GeV emission detected from such sub-luminous pulsars can be due to a lower altitude, lower-power accelerator gap.
Cognard Ismaël
Craig Helen A.
Johnston Scott
Kerr Matt
Romani Roger W.
No associations
LandOfFree
Sub-luminous gamma-Ray pulsars 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-luminous gamma-Ray pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sub-luminous gamma-Ray pulsars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-42014