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Cone Nebula Region
NGC281 - Pacman Nebula
Soul Nebula - IC1848
Heart Nebula - IC1805
Crescent Nebula and neighbours
  Eastern Veil and Pickering's Triangle.jpg -  Click      here   to enlarge    Eastern Veil and Pickering's Triangle       The Veil Nebula, also known as Cygnus Loop, in Cygnus constellation is a supernova remnant covering an area of 5 times the full Moon. Between 5000 to 8000 of years ago, a star exploded and its remnants have been expanded since then. The supernova lies at a distance of 1400 light-years approximately appearing to be rope like filaments. Visually it is difficult to see, but the aid of an OIII filter can help to distinguish the nebula from the sky background, due to part of the light emitted by the nebula is in this narrow band.   The foto was taken using narrowband Ha and [OIII] filters during two different nights. The night the Ha images were taken on a very clear night with quite good coditions. It has allowed us to go deep during the image post-processing revealing the dimmest parts of the nebula.    Source: Wikipedia and NASA/APOD   Lens: Megrez 72 APO + FF 0.8x   F/stop: 4.8   Exposure: Ha baader filter, 8 x 15 min;  and OIII 7x15min (unbinned)    Mount: Vixen Sphinx Deluxe    Camera: Artemis 4021    Guiding: Throught WO 66 f5.9 with Meade DSI and MaximDL software    Location:  Majada del Hombro, Huerta del Marquesado, Cuenca, Spain    Date:  July 31st and August 2nd 2008    Processing: Calibrated and aligned with DSS, stacked with MaximDL and postprocessed with PixInsight 1.2  
Norteamerica Nebula and Pelican
IC1396 and the elephant trunk
Rosette Nebula
Horse Head and neighbours
pelican_ic5070

 

Click here to enlarge

Eastern Veil and Pickering's Triangle

The Veil Nebula, also known as Cygnus Loop, in Cygnus constellation is a supernova remnant covering an area of 5 times the full Moon. Between 5000 to 8000 of years ago, a star exploded and its remnants have been expanded since then. The supernova lies at a distance of 1400 light-years approximately appearing to be rope like filaments. Visually it is difficult to see, but the aid of an OIII filter can help to distinguish the nebula from the sky background, due to part of the light emitted by the nebula is in this narrow band.

The foto was taken using narrowband Ha and [OIII] filters during two different nights. The night the Ha images were taken on a very clear night with quite good coditions. It has allowed us to go deep during the image post-processing revealing the dimmest parts of the nebula.

Source: Wikipedia and NASA/APOD

Lens: Megrez 72 APO + FF 0.8x

F/stop: 4.8

Exposure: Ha baader filter, 8 x 15 min; and OIII 7x15min (unbinned)

Mount: Vixen Sphinx Deluxe

Camera: Artemis 4021

Guiding: Throught WO 66 f5.9 with Meade DSI and MaximDL software

Location: Majada del Hombro, Huerta del Marquesado, Cuenca, Spain

Date: July 31st and August 2nd 2008

Processing: Calibrated and aligned with DSS, stacked with MaximDL and postprocessed with PixInsight 1.2

| 7/08/08 22:01
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