Three large H II regions and several fainter ones can be seen in the Carnegie Atlas of Galaxies images. Wikipedia ngc 5468 is a frontal spiral galaxy about 142 million light years away in the constellation Virgo. Wikipedia NGC 5468 is a frontal spiral galaxy in the constellation Virgo at a distance of about 142 million light years. It is located at a distance of about 140 million light years from Earth, which, given its apparent size, means that NGC 5468 has a diameter of about 110,000 light years.
Wikipedia NGC 5468 is a frontal spiral galaxy about 142 million light years away in the constellation Virgo. In the years since the galaxy’s discovery, astronomers have observed a number of supernova explosions in it. NGC 5468 – Intermediate Spiral Galaxy in the constellation Virgo is classified as an intermediate spiral (SABc) according to the Hubble and de Vaucouleurs morphological classification.
Which NGC is our galaxy?
Index The abbreviation NGC stands for “New General Catalogue” and is usually prefixed to a number in the catalogue, such as NGC 4258. At the distance given, the edge of the field shown corresponds to about 200,000 light years, about twice the size of the Milky Way. NGC 1 was first observed by Heinrich d’Arrest in 1860, when he tested the 11-inch refractor telescope at the Copenhagen Observatory. NGC 6744 (also known as Caldwell 10) is an intermediate spiral galaxy about 30 million light years away in the constellation Pavo (Peacock).
NASA’s Hubble Space Telescope captured this remarkable view of a perfectly edge-on galaxy, NGC 4013.
What is so special about the galaxy NGC 1052 DF2?
NGC 1052-DF2 is an ultra-diffuse galaxy (UDG) in the constellation Cetus, discovered during a wide-field survey of the NGC 1052 group with the Dragonfly Telephoto Array. AURA’s Space Telescope Science Institute in Baltimore, Maryland, manages Hubble’s science operations. In the second study, the team used the Keck Observatory’s Low Resolution Imaging Spectrometer (LRIS) to find another galaxy with no dark matter, named NGC 1052-DF4, or DF4 for short. The mystery surrounding the galaxy NGC 1052-DF2 deepens with each new revelation astronomers make with the Hubble Space Telescope.
When astronomers first observed this strange galaxy, they couldn’t believe it was missing the primary source of matter that holds it – dark matter.
What kind of galaxy is NGC 2775?
There is virtually no star formation in the central part of the galaxy. This is dominated by an unusually large and relatively empty galactic bulge, where all the gas was converted into stars long ago. The spiral nature of the fluffy galaxies contrasts with the large-scale spirals, which have distinct, well-defined spiral arms. The image below is of NGC 2775 from the Digitised Sky Survey 2 (DSS2 – see imprint), taken in the red channel. The galactic bulge is where all the gas in the galaxy was converted into stars when it first formed.
What type of galaxy is NGC 1705?
Figures 5 and 6 and Table 6 summarise and compare the results obtained with different models for NGC 1569, where the SFH and stellar yield can change in succession. They represent the building blocks from which more massive objects (spiral and elliptical galaxies) were later formed by merging and accretion. Time evolution of oxygen (top) and nitrogen-oxygen ratio (bottom) in the ISM of NGC 1705. Figures 5 and 6 and Table 6 summarise the results obtained with different models for NGC 1569, where SFH and stellar yields change sequentially. Time evolution of oxygen (upper panel) and nitrogen to oxygen (lower panel) in the ISM of NGC 1705.NGC 1705 is a peculiar lenticular galaxy and a blue compact dwarf galaxy (BCD) in the southern constellation Pictor, less than one degree east of Iota Pictoris, and is currently undergoing a starburst.