1E 0056.8-7154 RA 2000:   00:58:37.0 2 DEC2000: -71:35:48 2 Type:     PN Discovery paper ROSAT PSPC [c/s]: 0.29-0.35 9 17 NHgal [1021 cm-2]: 0.507

References:

1. Henize K.G., 1956, ApJS 2, 315 position
2. Aller L.H., Keyes C.D., 1987, ApJ 320, 159 position, UV spectrum
3. Wood P.R., Meatheringham S.J., Dopita M.A., Morgan D.H., 1987, ApJ 320, 178 optical diameter limit from Speckle imaging, OIII and H(beta) flux
4. Dopita M.A., Meatheringham S.J., 1991, ApJ 367, 115 photoionisation modelling of optical spectrum, nebular parameters
5. Meatheringham S.J., Dopita M.A., 1991, ApJ Suppl. 75, 407 optical line intensities, abundances, comparison with other PN
6. Wang Q., 1991, MNRAS 252, 47p Einstein X-ray data, spectrum, luminosity
7. Wang Q., Wu X., 1992, ApJ Suppl. 78, 391 SMC survey, discovery of soft and luminous X-ray spectrum
8. Brown T., Cordova F., Ciardullo R., Thompson R., Bond H., 1994, ApJ 422, 118 reanalysis Einstein data
9. Kahabka P., Pietsch W., Hasinger G., 1994, A&A 288, 538 ROSAT X-ray data on several SMC/LMC sources
10. Hughes J.P., 1994, ApJ 427, L25 variability ROSAT/Einstein
11. Heise J., van Teeseling A., Kahabka P., 1994, A&A 288, L45 WD atmosphere modelling of ROSAT data
12. Remillard R.A., Rappaport S., Macri L.M., 1995, ApJ 439, 646 ionisation nebula
13. van Teeseling A., Heise J., Kahabka P., 1996, IAU Symp. 165, eds J. van Paradijs et al., Kluwer Acad. Publ., p. 445 WD atmosphere modelling
14. Mürset U., Schild H., Vogel M., 1996, A&A 307, 516 optical spectrum, donor spectral type, IR photometry
15. Kahabka P., Pietsch W., 1996, A&A 312, 919 count rates, hardness ratio and spectral fit in summary table
16. Vassiliadis E., Dopita M.A., Meatheringham S.J., Bohlin R.C., Ford H.C., Harrington J.P., Wood P.R., Stecher T.P., Maran S.P., 1998, ApJ 503, 253 OIII image from HST
17. Kahabka P., Pietsch W., Filipovic M.D., Haberl F., 1999, A&A Suppl. 136, 81 SMC Survey, X-ray count rate
18. Stanghellini L., Blades J.C., S. J. Osmer S.J., Barlow M.J., Liu X.-W., 1999, ApJ 510, 687 HST images