Edge Rewrite
everything Source code View original
// HTMLRewriter · presentation

This page was redesigned at the edge.

Cloudflare fetched the original article and streamed it through HTMLRewriter to apply an entirely new visual system without rebuilding the source page.

// request.cf · coarse context

A page that knows where it met you.

Only coarse request metadata is shown. This demo does not display or persist visitor IP addresses.

Country
US
Cloudflare location
CMH
Connection
HTTP/2
Language
Not provided

Ray ID: a2202a0bcad51ef0

Jump to content

L183

Add links
From Wikipedia, the free encyclopedia
L183
Molecular cloud
L183 in different infrared wavelengths as imaged by the Spitzer Space Telescope
Observation data: J2000 epoch
Right ascension15h 54m 12.2s[1]
Declination−02° 49′ 42″[1]
Distance360[citation needed] ly
Apparent diameter75′[1]
ConstellationSerpens
DesignationsLDN 134N
See also: Lists of nebulae

L183 or L134N is a pre-stellar core in the constellation Serpens Cauda 360 light-years away. This massive accumulation of gas and dust was the interstellar object in which the phenomenon of coreshine was first investigated by astronomers and produced a new means of probing its previously opaque core.[2][3]

[edit]

References

[edit]
  1. 1 2 3 "LDN 183". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 24 September 2017.
  2. ↑ L183 (L134N) Revisited - L. Pagani, A. Bacmann et al.
  3. ↑ Charlotte Vastel, T.G Phillips, P Caselli, C Ceccarelli and L Pagani Deuterium enhancement in pre-stellar cores


Retrieved from "https://en.wikipedia.org/w/index.php?title=L183&oldid=1311609518"