Its shape is classified as SAbc, which means. Nearby type Ia supernovae like SN 2002fk in NGC 1309 are used by astronomers to calibrate distance measurements in the universe. Nearby Type Ia supernovae like SN 2002fk in NGC 1309 are used by astronomers to calibrate distance measurements in the Universe. This colour image shows stunning details of the face-up spiral galaxy catalogued as NGC 1309.
Observations of the recent supernova and Cepheid binaries in NGC 1309 are not just another pretty spiral galaxy, but also contribute to the calibration of the expansion of the Universe. If I saw NGC 1309 in a database or in a journal table, I wouldn’t give it a second glance. Refrain from using words like a, and, for, the, etc.
What is NGC in the Milky Way Galaxy?
NGC 6744 (also known as Caldwell 10) is an intermediate spiral galaxy about 30 million light years away in the constellation Pavo (Peacock). It is 6.5 million light years away from NGC 300, making it one of the Milky Way’s closer neighbouring galaxies. The Index Catalogue (IC) lists another 5,286 galaxies, nebulae and star clusters discovered between 1888 and 1907.NGC 6744 (also known as Caldwell 10) is an intermediate spiral galaxy about 30 million light years away in the constellation Pavo (Peacock). The Index Catalogue (IC) lists a further 5 286 galaxies, nebulae and star clusters discovered between 1888 and 1907. In 1888, the New General Catalogue (NGC) was published by the Royal Astronomical Society, listing 7 840 objects.
In this Hubble Space Telescope image, myriads of stars can be made out in the heart of nearby galaxy NGC 300, like grains of sand on a beach.
Does NGC 1705 form stars?
A fainter (ν= 0.05 Gyr- but long-lasting (Δt= 6 Gyr) SF episode is thought to have occurred between t= 5.55 and t= 11.55 Gyr, for which HST photometry does not provide detailed information. The central region of the small galaxy NGC 1705 shines with the light of thousands of young and old stars. This information and recent observations suggest that the SFH of most DIGs and BCDs is fairly continuous (Schulte-Ladbeck et al. Observational data support this by the chemical homogeneity of most star-forming galaxies, where the expected spatial variations in oxygen abundances are not observed, despite the presence of several massive clusters (Kobulnicky & Skillman 1997, 199.
What kind of galaxy is NGC 1232?
The following image is of NGC 1232 from the Digitized Sky Survey 2 (DSS2 – see imprint), taken in the red channel. This deviation of the arms is probably due to gravitational encounters with NGC 1232A as it orbits the larger spiral. We constructed the luminosity function for NGC 1232 using the same criteria used by previous authors (e.g. It can be seen that the luminosity function in NGC 1232 shows a break in the slope, with the fainter H ii regions showing a flatter slope compared to the more luminous objects.
We have also constructed the magnitude distribution function and found that NGC 1232, like most galaxies, follows an exponential law.
Because the arc is shaped like a stretched-out umbrella, this galaxy is called the “Umbrella Galaxy”. Unlike most spiral galaxies of the Virgo Cluster, NGC 4651 is rich in neutral hydrogen, which also extends beyond the optical disk, and its star formation is typical of a galaxy of its type. Unlike most spiral galaxies of the Virgo Cluster, NGC 4651 is rich in neutral hydrogen that also extends beyond the optical disk, and its star formation is typical of a galaxy of its type. The photo shows the galaxy NGC 4651 in all its glory, with its extended spiral arms clearly visible and its brightly shining galactic centre.
Astronomers suspect that this cosmic screen is made up of stellar streams, the trails of stars stripped from a smaller galaxy nearby that engulfed NGC 4651 in the distant past. However, fine processing of the image taken by a large-calibre telescope revealed the slender arms extending outwards at either end of the galactic disk and the faint circular arc extending beyond the arms.
What kind of galaxy is NGC 4651?
Studies of the distribution of neutral hydrogen with radio telescopes reveal distortions in the outer regions of NGC 4651 and a clump of gas associated with a dwarf galaxy that may have been formed in the event that produced the aforementioned stellar streams. However, fine processing of the image taken with a large-calibre telescope found the slender arms extending outwards at both ends of the galactic disk and the faint circular arc extending beyond the arms. Unlike most spiral galaxies of the Virgo Cluster, NGC 4651 is rich in neutral hydrogen that also extends beyond the optical disk, and its star formation is typical of a galaxy of its type.
What is NGC in the Milky Way Galaxy?
Although the stream of superheated gas emanating from NGC 4666 is truly enormous, stretching tens of thousands of light-years, it is not visible in this image. The Index Catalogue (IC) lists a further 5,286 galaxies, nebulae and star clusters discovered between 1888 and 1907. Although the stream of superheated gas emanating from NGC 4666 is truly enormous, stretching over tens of thousands of light years, it is not visible in this image. The Index Catalogue (IC) lists a further 5 286 galaxies, nebulae and star clusters discovered between 1888 and 1907, as well as at least one distorted companion galaxy (NGC 6744A) that superficially resembles one of the Magellanic Clouds. This, together with the evidence of a very faint thread of material extending between Stephan’s Quintet and NGC 7331, suggests an earlier gravitational interaction.
In this Hubble Space Telescope image, myriads of stars can be made out in the heart of the nearby galaxy NGC 300, like grains of sand on a beach.
