1995A&A...297..828B


Query : 1995A&A...297..828B

1995A&A...297..828B - Astronomy and Astrophysics, volume 297828-834 (1995/5-3)

A model of the planetary nebula NGC 2440.

BAESSGEN M., DIESCH C. and GREWING M.

Abstract (from CDS):

A 2-dimensional cylindrically symmetric ionisation model of the planetary nebula NGC 2440 is presented. The gridsize with which the model has been calculated has been adapted to match the spatial resolution of monochromatic CCD-images obtained in several emission lines. The comparison between "real" images and "model" images yields an accurate simulation of the ionisation structure. From our models we also determined a consistent set of physical quantities of NGC 2440. Our resulting distance is 500pc, the central star temperature and luminosity are 125000K and 250L☉ respectively.

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Journal keyword(s): planetary nebulae: individual: NGC 2440 - planetary nebulae: general

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 40 PN 00 13 01.0170097248 +72 31 19.033338720   11.63 11.46     [WC8] 632 2
2 NGC 2440 PN 07 41 55.34603 -18 12 30.4117   11.469 10.104     ~ 665 2
3 NGC 3132 PN 10 07 01.7656422504 -40 26 11.130553032   10.14 10.01     A2V 423 1

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