NGC 2024
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NGC 2024 far-infrared and radio molecular observations by

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Published by National Aeronautics and Space Administration, Ames Research Center in Moffett Field, Calif .
Written in English


  • Infrared technology,
  • Molecular spectra

Book details:

Edition Notes

Other titlesN.G.C. two thousand twenty four
StatementHarley A. Thronson, Jr. ... [et al.]
SeriesNASA technical memorandum -- 85954
ContributionsThronson, Harley A, Ames Research Center
The Physical Object
Pagination1 v.
ID Numbers
Open LibraryOL17977476M

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  NGC , The Flame Nebula - posted in Sketching: Often overlooked, NGC gets no respect. As an emission nebula in the constellation Orion it is overshadowed by the majesty of M In wide-field photographs attention is inevitably drawn to that dramatic dark inclusion that is the Horsehead Nebula. In the eyepiece it is nearly overwhelmed by the . Get this from a library! The dense molecular ridge in NGC [Tomomi Watanabe; Saint Mary's University (Halifax, N.S.). Astronomy and Physics Department.; Saint . NGC is a reflection nebula situated to the south of the Flame Nebula (NGC ) and at the edge of the H ii region IC , which also contains the Horsehead Nebula (Barnard 33).   Horsehead and Flame Nebulas in Orion. The Flame Nebula is near the star Alnitak in Orions belt. Picture is made up of 70 60sec exposures with a QSI cs color camera cooled to degrees centigrade.

  Horsehead and the NGC - posted in DSLR & Digital Camera Astro Imaging & Processing: This was shot right beside of the 90% moon last weekend. SW 80 ed, nikon d(fullspectrum & coldfinger cooled) sensor temp -5c*. IDAS lps-d1 filter. Integration time 4h. 10min frames. Mount eq-5 hyper mod. Only stacked in pixinsight and processed in PS. OCLC Number: Notes: "Airborne Astronomy Program, Medium Altitude Missions Branch, Preprint series " "May "--Cover. "N"--Microfiche header. NGC is a rich and moderately concentrated, with Trumpler class III1r, open cluster. The brightest stars of the cluster are of magnit the brightest being of magnitude The cluster has members down to 15th magnitude. The main sequence turn off is at magnitude and there are few red giants llation: Orion. The image found on this page (only) is licensed under a Creative Commons Attribution-ShareAlike United States License. Although larger versions of this image are available, they are NOT to be used without the expressed permission of Adam Block.

5oz silver hot springs 5oz silver 25c hot springs ms 5oz silver hot springs 5oz silver 25c hot springs ms shop! shop! updated: 4/23/ 25c: ms: 8, New book chronicles the space program; Astro stuff galore at the Swap and Sell; Brian May and David Eicher to give talks in London, Bath, and Amsterdam Tags: Horsehead Nebula, Ic , ngc , Flame Nebula, B The NGC Chandra X-Ray Point Source Catalog contains the results of a sensitive 76 ks Chandra observation of the young stellar cluster in NGC , lying at a distance of ~ pc in the Orion B giant molecular cloud. Previous infrared observations have shown that this remarkable cluster contains several hundred embedded young stars, most of. Astronomers have studied two star clusters using data from Chandra and infrared telescopes, and results show that the simplest ideas for the birth of these clusters cannot work.