Tag Archives: NGC 2237

The Rosette Nebula, NGC 2237

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The Rosette Nebula (also known as Caldwell 49) is a large, circular H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the stars of the cluster having been formed from the nebula’s matter.

The complex has the following NGC designations:

NGC 2237 – Part of the nebulous region (Also used to denote whole nebula)
NGC 2238 – Part of the nebulous region
NGC 2239 – Part of the nebulous region (Discovered by John Herschel)
NGC 2244 – The open cluster within the nebula (Discovered by John Flamsteed in 1690)
NGC 2246 – Part of the nebulous region
The cluster and nebula lie at a distance of some 5,200 light-years from Earth (although estimates of the distance vary considerably, down to 4,900 light-years.[3]) and measure roughly 130 light years in diameter. The radiation from the young stars excites the atoms in the nebula, causing them to emit radiation themselves producing the emission nebula we see. The mass of the nebula is estimated to be around 10,000 solar masses.

It is believed that stellar winds from a group of O and B stars are exerting pressure on interstellar clouds to cause compression, followed by star formation in the nebula. This star formation is currently still ongoing.

A survey of the nebula with the Chandra X-ray Observatory in 2001 has revealed the presence of very hot, young stars at the core of the Rosette Nebula. These stars have heated the surrounding gas to a temperature in the order of 6 million kelvins causing them to emit copious amounts of X-rays.

Imaging telescopes or lenses: Takahashi FSQ 106ED ED III
Imaging cameras: SBIG STT-8300M
Mounts: GTD Gemini Telescope Design – Hungary G53F
Guiding telescopes or lenses: Takahashi FSQ 106ED ED III
Guiding cameras: SBIG STT-8300M
Focal reducers: Takahashi 0.75x FSQ F/3,6 Riduttore Focale TAKA
Software: Pixinsight Core 1.8
Resolution: 2635×2245
Dates: Dec. 12, 2014
Frames: 45×600″
Integration: 7.5 hours
Avg. Moon age: 19.90 days
Avg. Moon phase: 73.05%
RA center: 97.942 degrees
DEC center: 5.015 degrees
Orientation: -97.003 degrees
Field radius: 1.401 degrees

Author: Davide Fiore

Rosette Nebula and open cluster NGC 2244

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The Rosette Nebula (also known as Caldwell 49) is a large, circular H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the starsof the cluster having been formed from the nebula’s matter.
The cluster of stars is visible in binoculars and quite well seen in small telescopes while the nebula itself is more difficult to spot visually and requires a telescope with a low magnification. A dark site is a must to see it. Photographically the Rosette Nebula is easier to record and it is the only way to record the red color which is not seen visually.

Imaging telescopes or lenses: Orion ED80
Imaging cameras: SBIG ST-10 XME
Mounts: Mountain Instruments MI-250
Guiding telescopes or lenses: Astro-Tech 8x50mm Finder Guidescope
Guiding cameras: Starlight Xpress Lodestar
Software: Main Sequence Software Sequence Generator Pro, PHD guiding, PixInsight
Filters: Astrodon Ha 5nm, Astrodon SII 5nm
Accessories: Astro-Tech 2″ Field Flattener, Shoestring Astronomy FCUSB, SBIG CFW 10, Moonlite CF 2″ focuser with high resolution stepper
Dates: April 7, 2013
Frames:
Astrodon Ha 5nm: 4×600″ -30C bin 1×1
Astrodon SII 5nm: 4×600″ -30C bin 1×1
Integration: 1.3 hours
Darks: ~20
Flats: ~20
Bias: ~200

Autor: Chris Madson

AstroPhotography of the day by SPONLI

13 February 2014

We select the best works of amateur astrophotographers with details of equipment, shooting processing etc.

NGC 2237: The Rosette Nebula

75c4ee7b553598c697c33965e4705772.1824x0_q100_watermark
The Rosette Nebula (also known as Caldwell 49) is a large, circular H II region located near one end of a giant molecular cloud in the Monoceros region of the Milky Way Galaxy. The open cluster NGC 2244 (Caldwell 50) is closely associated with the nebulosity, the starsof the cluster having been formed from the nebula’s matter. A survey of the nebula with the Chandra X-ray Observatory in 2001 has revealed the presence of very hot, young stars at the core of the Rosette Nebula. These stars have heated the surrounding gas to a temperature in the order of 6 million kelvins causing them to emit copious amounts of X-rays.

Imaging telescopes or lenses: Takahashi TOA-130
Imaging cameras: FLI ML 11002
Mounts: Astro-Physics Mach 1 GTO
Guiding telescopes or lenses: Takahashi TOA-130
Guiding cameras: Starlight Xpress Lodestar
Software: Adobe Photoshop CS6, Main Sequence Software Sequence Generator Pro, CCDStack2
Filters: Astrodon Narrowband Set (Ha OIII SII)
Accessories: 67 Field Flattener
Dates: Jan. 11, 2014
Frames: 58×1200″

Autor: Mark Striebeck

AstroPhotography of the day by SPONLI

30 January 2014

We select the best works of amateur astrophotographers with details of equipment, shooting processing etc.