NGC 3199:  A View in LRGB Completed by Ha, O3 and S2 Narrow Band Data, Fernando

NGC 3199: A View in LRGB Completed by Ha, O3 and S2 Narrow Band Data

NGC 3199:  A View in LRGB Completed by Ha, O3 and S2 Narrow Band Data, Fernando

NGC 3199: A View in LRGB Completed by Ha, O3 and S2 Narrow Band Data

Equipment

Loading...

Acquisition details

Loading...

Description

Distant from Earth 11 736 light years in the southern constellation of Carina, NGC 3199 is classed as a diffuse nebula, embedded with a highly assymetric Wolf-Rayet star close to the center of the ring. The nebula is about 75 light-years across.

A Wolf-Rayet star is hot, short-lived and generates an intense stellar wind. The one in NGC 3199, as mentioned, has a highly asymmetric morphology, with a very bright hemisphere near the exciting star HD 89358 and a much fainter and more extended other hemisphere.

This nebula is modeled in terms of the distorted bubble produced by a moving star blowing a strong stellar wind into a surrounding uniform interstellar medium.

This description is an outine of the article found in:

http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1989A%26A...226..270D&defaultprint=YES&filetype=.pdf

The image is a LRGB standard enhanced by narrow band data from captures of 12 subframes of 20 minutes for each channel (Ha, O3 e S2).

The subs of LRGB followed the sequence showed below:

Lum: 10x900sec bin1x1

RGB: 10x600sec bin2x2

Set-up:

Scope: Esprit 120 f/7

Mount: CGE-Pro

Camera: ST8300M

OAG and Filter Wheel: SBIG 8300

Guider CCD: Lodestar

Darks, bias and Flats applied

Comments

Histogram

NGC 3199:  A View in LRGB Completed by Ha, O3 and S2 Narrow Band Data, Fernando