1997A&A...317...99K

Query : 1997A&A...317...99K

1997A&A...317...99K - Astronomy and Astrophysics, volume 31799 (1997/1-1)

The TeV γ-ray visibility of Geminga-like pulsars.

KAUL R.K.

Abstract (from CDS):

It is shown that, while the number of Geminga-like pulsars in the Galaxy may be ∼103, the prospects of detecting TeV gamma-ray signals from them are not very encouraging. Arguments are presented to show that Geminga-like pulsars having periods in the range 200-500ms, surface magnetic fields >1012Gauss and preferentially located within ∼2kpc of the earth may be able to produce detectable TeV gamma-ray signals.

Abstract Copyright: ∼

Journal keyword(s): pulsars: individual: Geminga - pulsars: general - gamma rays: theory

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 PSR B0114+58 Psr 01 17 38.661 +59 14 38.39           ~ 96 0
2 PSR B0355+54 Psr 03 58 53.7165 +54 13 13.727           ~ 465 1
3 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
4 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
5 PSR J0633+1746 Psr 06 33 54.153 +17 46 12.91           ~ 1308 0
6 PSR B1055-52 Psr 10 57 59.0450 -52 26 56.330           ~ 757 0
7 PSR B1509-58 Psr 15 13 47.6 -59 07 54     13.06     ~ 879 1
8 PSR B1706-44 Psr 17 09 42.62000 -44 29 12.0000     13.30     ~ 670 1

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