Table A.1: A comparison of previously known shells (Heiles 1979) and our identifications. The first column gives the names of the structures, the second one gives dimensions as published by Heiles, the third column gives our dimensions ($\Delta l$, $\Delta b$, $\Delta v$).
Name Heiles this paper
  ${\rm deg}^2 \ {\rm km~s^{-1}}$ ${\rm deg}^2 \ {\rm km~s^{-1}}$
GS090+02-115 $4\times 4\times 16$ $3\times 4\times 12$
GS091-04-69 $9\times 10\times 28$ $3\times 5\times 33$
GS091+02-101 $4\times 3\times 12$ $4\times 4\times 33$
GS108-04-23 $5\times 11\times 24$ $7\times 14\times 20$
GS128+01-105 $7\times 6\times 4$ $11\times 5\times 16$
GS148-01+15 $4\times 4\times 4$ $3\times 5\times 10$
GS152-04-41 $4\times 4\times 12$ $11\times 9\times 12$
GS095+04-113 $10\times 5\times 20$ $10\times 6\times 21$
GS139-03-69 $18\times 10\times 28$ $13\times 6\times 22$


Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Data
3 Searching algorithm
4 Other automatic searches for H I shells
5 H I shells in the Leiden-Dwingeloo survey
6 Distribution of shells in the Milky Way from distance effect removed (DER) samples
7 Filling factor of H I shells
8 Summary
References
Online Material
Appendix A: A comparison with other lists
List of tables
List of figures