by APOD Robot » Wed Mar 25, 2020 4:05 am
Star Forming Region S106
Explanation: Massive star IRS 4 is beginning to spread its wings. Born only about 100,000 years ago, material streaming out from this
newborn star has formed the nebula dubbed Sharpless 2-106 Nebula (S106),
featured here. A large disk of
dust and gas orbiting Infrared Source 4 (IRS 4), visible in brown near the image center, gives the nebula an
hourglass or
butterfly shape.
S106 gas near IRS 4 acts as an
emission nebula as it emits light after being
ionized, while
dust far from
IRS 4 reflects light from the central star and so acts as a
reflection nebula. Detailed inspection of a relevant
infrared image of S106 reveal hundreds of low-mass
brown dwarf stars lurking in
the nebula's gas. S106 spans about 2
light-years and lies about 2000 light-years away toward the
constellation of the Swan (
Cygnus).
[url=https://apod.nasa.gov/apod/ap200325.html] [img]https://apod.nasa.gov/apod/calendar/S_200325.jpg[/img] [size=150]Star Forming Region S106[/size][/url]
[b] Explanation: [/b] Massive star IRS 4 is beginning to spread its wings. Born only about 100,000 years ago, material streaming out from this [url=https://science.nasa.gov/astrophysics/focus-areas/how-do-stars-form-and-evolve/]newborn star[/url] has formed the nebula dubbed Sharpless 2-106 Nebula (S106), [url=https://www.flickr.com/photos/163350986@N06/43790342142/in/dateposted-public/]featured here[/url]. A large disk of [url=https://apod.nasa.gov/apod/ap030706.html]dust[/url] and gas orbiting Infrared Source 4 (IRS 4), visible in brown near the image center, gives the nebula an [url=https://apod.nasa.gov/apod/ap150510.html]hourglass[/url] or [url=https://apod.nasa.gov/apod/ap141001.html]butterfly[/url] shape. [url=https://www.mpia-hd.mpg.de/IRCAM/OPRIME/Gallery/ASTRO/S106.html]S106[/url] gas near IRS 4 acts as an [url=https://apod.nasa.gov/apod/emission_nebulae.html]emission nebula[/url] as it emits light after being [url=https://en.wikipedia.org/wiki/Ionization]ionized[/url], while [url=https://ned.ipac.caltech.edu/level5/Mathis/Mathis1.html]dust[/url] far from [url=https://ui.adsabs.harvard.edu/abs/2009AJ....137.3149S/abstract]IRS 4[/url] reflects light from the central star and so acts as a [url=https://apod.nasa.gov/apod/reflection_nebulae.html]reflection nebula[/url]. Detailed inspection of a relevant [url=https://apod.nasa.gov/apod/ap111107.html]infrared image[/url] of S106 reveal hundreds of low-mass [url=https://en.wikipedia.org/wiki/Brown_dwarf]brown dwarf stars[/url] lurking in [url=https://ui.adsabs.harvard.edu/abs/1998AJ....116.1868B/abstract]the nebula's[/url] gas. S106 spans about 2 [url=http://starchild.gsfc.nasa.gov/docs/StarChild/questions/question19.html]light-years[/url] and lies about 2000 light-years away toward the [url=https://en.wikipedia.org/wiki/Constellation]constellation[/url] of the Swan ([url=https://en.wikipedia.org/wiki/Cygnus_(constellation)]Cygnus[/url]).
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