Abstract
Several new supernova remnants (SNRs) have been recently identified from sensitive radio continuum surveys of the Galactic plane. The limit in surface brightness is about ∫1GHz = 2·10−22 [W/m2 Hz sr]. In comparison with previously known SNRs, which are in their majority much brighter, we reexamine the distribution of SNRs in the first Galactic quadrant and some statistical properties.
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Reich, W., Fürst, E., Reich, P., Junkes, N.: 1986, in Supernova Remnants and the Interstellar Medium, IAU Coll. 101, eds. R.S. Roger and T.L. Landecker, Cambridge University Press, p. 293
Junkes, N., Fürst, E., Reich, W.: 1988, this volume
Reich, W., Fürst, E., Altenhoff, W.J., Reich, P., Junkes, N.: 1985, Astron. Astrophys. 151, L10
Reich, W., Junkes, N., Fürst, E.: 1988, this volume
Fürst, E., Hummel, E., Reich, W., Sofue, Y., Sieber, W., Reif, K., Dettmar, R.J.: 1988, Astron. Astrophys., submitted
Milne, D.: 1979, Australian J. Phys. 32, 83
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© 1988 Springer-Verlag
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Reich, W., Fürst, E. (1988). Statistical properties of recently new identified supernova remnants. In: Kundt, W. (eds) Supernova Shells and Their Birth Events. Lecture Notes in Physics, vol 316. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-50435-4_7
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DOI: https://doi.org/10.1007/3-540-50435-4_7
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