The correlation analysis on Comptel 26Al with SNR and W-R stars.

Details The correlation analysis on Comptel 26Al with SNR and W-R stars. The correlation analysis on Comptel 26Al with SNR and W-R stars.

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997jbnun..33..371l&link_type=abstract

Journal of Beijing Normal University (Natural Sciences), Vol. 33, No. 3, p. 371 - 375

Astronomy and Astrophysics

Astronomy

Gamma Rays: Wolf-Rayet Stars, Gamma Rays: Supernovae, Correlation Analysis: Gamma-Ray Astronomy

Scientific paper

The current viewpoint of the possible sources of 26Al is massive stars, Wolf-Rayet stars, AGB stars, supernovae of Type II and Ib and novae. Taking advantage of the data processing results of the Comptel observations, the correlation of the 1.8 MeV γ-ray with the SMI and the W-R stars is analyzed. The goodness-of-fit of their distributions along the Galactic longitude is studied. According to the results of K-S tests, the W-R stars and 1.8 MeV come from the same distribution (α = 0.10). The correlation analysis also shows that the W-R stars are correlative fairly to the 1.8 MeV.

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