Identification of the nebula G70.7 + 1.2 as a bow shock powered by a pulsar/Be-star binary-Reference-Cited by-同舟云学术

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Identification of the nebula G70.7 + 1.2 as a bow shock powered by a pulsar/Be-star binary

Published:1992-11 Issue:6400 Volume:360 Page:139-141
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Kulkarni S. R.,Vogel S. N.,Wang Z.,Wood D. O. S.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/360139a0.pdf

Reference19 articles.

1. Reich, W., Fürst, E., Stuffen, P., Reif, K. & Haslam, C. G. T. Astr. Astrophys. Suppl. 58, 197–248 (1984).

2. Green, D. A., Mon. Not. R. astr. Soc. 216, 691–700 (1985).

3. Reich, W., Fürst, E., Altenhoff, W. J., Reich, P. & Junkes, N. Astr. Astrophys. 151, L10–L12 (1985).

4. de Muizon, M., Strom, R. G., Oort, M. J. A., Claas, J. J. & Braun, R. Astr. Astrophys. 193, 248–264 (1988).

5. Van Buren, D., Mac Low, M.-M., Wood, D. O. S. & Churchwell, E. Astrophys. J. 353, 570–578 (1990).

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