Visitors Now:
Total Visits:
Total Stories:
Profile image
By Anne's Astronomy News
Contributor profile | More stories
Story Views

Now:
Last Hour:
Last 24 Hours:
Total:

Anne’s Image of the Day: Emission Nebula N214C

Friday, September 20, 2013 7:57
% of readers think this story is Fact. Add your two cents.

(Before It's News)

read more at Anne’s Astronomy News http://annesastronomynews.com/

September 20, 2013

N214C, an emission nebula in the LMC

N214C, an emission nebula in the LMC

Image Credit: ESO

N214C is an emission nebula of approximately 160 x 170 light-years across located within the Large Magellanic Cloud, a small satellite of the Milky Way that lies some 163,000 light-years away from Earth in the constellation of Dorado. It is part of the H II region N214, and is a noteworthy region of ongoing star formation.

Toward the middle of this star-forming (H II) region lies a tight cluster of stars named Sk −71◦51. This cluster contains at least 6 bright, massive stars, including the region’s brightest and hottest star, and probably hundreds of lower mass stars. These cluster stars are illuminating the nebula.

Some 50 light-years north of this cluster lies a striking compact Pac-Man-like blob of ionized gas, that may have resulted from massive star formation. This spherical structure of about four light-years across is split into two lobes by a dust lane which runs along an almost north-south direction.

In the gas blob astronomers discovered an impressively-strong infrared source, which means that a tremendous heat source must exist within it. Estimates indicate this infrared source is about 200,000 times more luminous than our own Sun, what means that the source is probably a very massive star that weighs about 40 times the mass of the Sun. Another explanation for the bright infrared light source could be that a 100-solar-mass star is currently being produced within the blob, but has not come out of its birth cocoon yet.

Another notable area of N214C is its south-eastern border (at the bottom left of this image), which is suggesting that this reddened H II region, where new stars are being born, is in contact with a molecular cloud in that direction.

This composite six-colour image, taken with the ESO NTT/SuSI2, results from the co-addition of several individual exposures taken through various narrow and broadband filters. North is up and east to the left.

n/a



Source: http://annesastronomynews.com/annes-image-of-the-day-emission-nebula-n214c/

Report abuse

Comments

Your Comments
Question   Razz  Sad   Evil  Exclaim  Smile  Redface  Biggrin  Surprised  Eek   Confused   Cool  LOL   Mad   Twisted  Rolleyes   Wink  Idea  Arrow  Neutral  Cry   Mr. Green

Top Stories
Recent Stories

Register

Newsletter

Email this story
Email this story

If you really want to ban this commenter, please write down the reason:

If you really want to disable all recommended stories, click on OK button. After that, you will be redirect to your options page.