Drfrancisco dias User talk: In a supernova, SN G, was observed which is the only supernova in this galaxy to be recorded so far. Madore NED and collaborator. This file contains additional information, probably added from the digital camera or scanner used to create or digitize it. The arms are also very rich in clouds of interstellar dust, seen as dark patches and streaks silhouetted against the starlight. But, strangely enough, there is no direct evidence for a supermassive black hole in the center of NGC
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It is a flocculent spiral galaxywith short nngc of spiral structure but without the dramatic well-defined spiral arms of a grand design spiral.
NGC 4414, a dusty spiral galaxy in Coma Berenices
Commons is a freely licensed media file repository. The arms are also very rich in clouds of interstellar dust, seen as dark patches and streaks silhouetted against the starlight.
The end result is a stunning full-color look at the entire dusty spiral galaxy. Wendy Freedman of the Observatories of the Carnegie Institution of Washington, observed this galaxy on 13 different occasions over the course of ngcc months.
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Dust lanes in Spiral Galaxy NGC
Jun 3, Ngv Use: NGC is an unbarred spiral galaxy about 62 million light-years away in the constellation Coma Berenices. The image is 2. If you have an image of similar quality that can be published under a suitable copyright licensebe sure to upload it, tag it, and nominate it. You can help Wikipedia by expanding it. New General Catalogue to GalaxyList of galaxies. The following other wikis use this file: View more global usage of this file.
In other projects Wikimedia Commons. This file contains additional information, probably added from the digital camera or scanner used to create or digitize it. In a supernovaSN G, was observed and was the only supernova in this galaxy to be recorded until June 7, when SN df was discovered at Magnitude Retrieved 25 November Anne’s Astronomy News in Dutch.
NGC – Wikipedia
Wendy Freedman of the Observatories of the Carnegie Institution of Washington, observed this galaxy on 13 different occasions over the course of two months. The outer spiral arms are considerably bluer due to the ongoing formation of young, blue stars — the brightest of which can be seen individually — between 414 is what appears to be a Luminous Blue Variable.
File:NGC 4414 (NASA-med).jpg
The arms are also very rich in clouds of interstellar dust, seen as dark patches and streaks silhouetted against the starlight. Width 1, 414 Height 1, px Bits per component 8 8 8 Compression scheme Uncompressed Pixel composition RGB Image data location 3, Number of components 3 Number of rows per 441 1, Bytes per compressed strip 7, Data arrangement chunky format.
From Wikipedia, the free encyclopedia. Inthe Hubble Heritage Team revisited NGC and completed its portrait by observing the other half with the same filters as were used in SA rs c .
If you have a different image of similar quality, be sure to upload it using the proper free license tagadd it to a relevant article, and nominate it. Results for NGC NGC also known as UGC is a massive unbarred spiral galaxy of some 56, light-years in diameter, located about