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1997ApJ...487L..65Y - Astrophys. J., 487, L65-L68 (1997/September-3)
Very high energy gamma rays from the Vela pulsar direction.
YOSHIKOSHI T., KIFUNE T., DAZELEY S.A., EDWARDS P.G., HARA T., HAYAMI Y., KAKIMOTO F., KONISHI T., MASAIKE A., MATSUBARA Y., MATSUOKA T., MIZUMOTO Y., MORI M., MURAISHI H., MURAKI Y., NAITO T., NISHIJIMA K., ODA S., OGIO S., OHSAKI T., PATTERSON J.R., ROBERTS M.D., ROWELL G.P., SAKO T., SAKURAZAWA K., SUSUKITA R., SUZUKI A., TAMURA T., TANIMORI T., THORNTON G.J., YANAGITA S. and YOSHIDA T.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Gamma Rays: Observations - ISM: Individual Name: Vela Supernova Remnant (Vela SNR) - ISM: Magnetic Fields - Stars: Pulsars: Individual Name: Vela Pulsar - ISM: Supernova Remnants
Simbad objects: 5
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