NGC 625 is a dwarf barred spiral galaxy about 12.7 Mly away in the constellation Phoenix. It was discovered on 2 September 1826 by Scottish astronomer James Dunlop. [3] NGC 625 is a member of the Sculptor Group. [4]

NGC 625 is a Barred Spiral Galaxy in the Phoenix constellation. NGC 625 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its visual magnitude of 11.25, NGC 625 is visible with the help of a telescope having an aperture of 6 inches (150mm) or more.

NGC 625 is a barred spiral galaxy. It is about 12.7 million light years distant and has an apparent magnitude of 11.7. The galaxy is a member of the Sculptor Group, a loose group of galaxies located near the south galactic pole in the constellations Sculptor and Cetus .

< NGC List NGC 625. NGC 625 is a barred spiral galaxy located in the constellation of Phoenix. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 625:

Sep 19, 2003 · NGC 625 has a well-defined radial stellar population gradient, evidenced by a central concentration of young MS stars and an RGB/AGB ratio that increases with galactocentric distance. The prominent AGB is very red, and RGB stars are detected far from the central star forming regions.

NGC 625 has a well-defined radial stellar population gradient, evidenced by a central concentration of young main-sequence stars and a red giant branch (RGB)/asymptotic giant branch (AGB) ratio that increases with galactocentric distance.

NGC 625 has a well-defined radial stellar population gradient, evidenced by a central concentration of young main sequence stars and an RGB/AGB ratio that increases with galactocentric distance. The prominent AGB is very red, similar to the population found in the Local Group dIrr NGC 6822.

Apr 30, 2004 · We present new multi-frequency radio continuum imaging of the dwarf starburst galaxy NGC 625 obtained with the Very Large Array. Data at 20, 6, and 3.6 cm reveal global continuum emission dominated by free-free emission, with only mild synchrotron components.

See if you can find the NGC 625, a spiral galaxy located in the constellation Phoenix.

Sep 14, 2004 · We present new FUSE spectroscopy of the dwarf starburst galaxy NGC 625. These observations probe multiple phases of the interstellar medium, including the coronal, ionized, neutral and molecular gas. This nearby (D = 3.9 +/- 0.2 Mpc) system shows a clear detection of outflowing coronal gas as traced by OVI 1032 Angstrom absorption.