by Diego Barucco

IC 1747

J2000
RA: 01h 57m 35.59s
Dec: +63 ° 19' 18.8"
Mag.13,60
Surface bright: 10,02
Dim.: 13"
Central star: 15,40 (var)
Constellation: Cassiopea

Discovery: Williamina Fleming, 1905
Distance: 2,93 kpc
Radius: 0,093 pc

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IC 1747 is a very interesting PN even with some difficulties of visual observation. In 8" telescopes it shows a vague anular shape at high magnifications, in which brightness lacks of homogeneity. Infact, a bright arch is visible toward N direction, and a deeper observation could reveal another condensation opposite to the first (toward S). Central star hardly emerges among gases of this nebula.
Astronomical researches haven't been continuous during past years, and it has not been possible yet to resolve some doubts on its morphology: studies carried on in '80s show a bipolar-toroid structure, with its polar axis toward us, so that we can observe its ring coinciding the equatorial toroid.
Recent studies underlined the presence of a faint asymmetrical halo, outside the main nebula, noticeable only with long exposure Halpha survey.

Interesting level: ****

Bibliography
The IUE Spectra of Three Optically Narrow-Line O VI Planetary Nebulae: NGC 1501, IC 1747, and IC 1297 - Feibelman, Walter A. - The Astrophysical Journal Supplement Series, Volume 119, Issue 2, pp. 197-205 (1998).

The evolution of planetary nebulae. III - Position-velocity images of butterfly-type nebulae - Icke, Vincent; Preston, Heather L.; Balick, Bruce - Astronomical Journal (ISSN 0004-6256), vol. 97, Feb. 1989, p. 462-475, 618-625. Research supported by the National Optical Astronomy Observatories and Digital Equipment Corp.


English traslation: Renzo Ruisi

Update: Tuesday, April 6, 2010 8:54 PM

 

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