
NGC 428 - Wikipedia
NGC 428 is a barred spiral galaxy in the constellation of Cetus (The Sea Monster), with its spiral structure distorted and warped, possibly the result of the collision of two galaxies. [3] There appears to be a substantial amount of star formation occurring within NGC 428 and it lacks well defined arms — a telltale sign of a galaxy merger. [ 3 ]
NGC 428 - 维基百科,自由的百科全书
ngc 428 是鲸鱼座的一個星系。 维基共享资源上的相關多媒體資源:ngc 428. ned – ngc 428; seds – ngc 428; simbad – ngc 428; vizier – ngc 428
Hubble Sees a “Mess of Stars” - Science@NASA
2015年8月14日 · Bursts of pink and red, dark lanes of mottled cosmic dust, and a bright scattering of stars — this NASA/ESA Hubble Space Telescope image shows part of a messy barred spiral galaxy known as NGC 428. It lies approximately 48 million light-years away from Earth in the constellation of Cetus (The Sea Monster).
A mess of stars - ESA/Hubble
2015年8月10日 · Bursts of pink and red, dark lanes of mottled cosmic dust, and a bright scattering of stars — this NASA/ESA Hubble Space Telescope image shows part of a messy barred spiral galaxy known as NGC 428. It lies approximately 48 million light-years away from Earth in the constellation of Cetus (The Sea Monster).
NGC428 - 百度百科
NGC428是鲸鱼座的棒旋星系,距离地球大约4800万光年。 从整体来看,这一星系显得非常扭曲、混乱。 科学家推测,这可能是两个星系碰撞交织而形成的结果。
Hubble Space Telescope Observes Barred Spiral NGC 428
2015年8月10日 · NGC 428, also known as LEDA 4367 or UGC 763, is a barred spiral galaxy located in the constellation Cetus. It was discovered by the British astronomer Sir William Herschel in December 1786. The galaxy is approximately 45,000 light-years across. It has an apparent magnitude of 11 and lies at a distance of 37 million light-years from Earth.
NGC 428 - NOIRLab
2014年2月25日 · NGC 428 is approximately 70 million light years away. Its distorted shape leads astronomers to think that this galaxy may have absorbed another galaxy in its recent history. The many starforming regions and bright blue star clusters hint …
NGC 428 - Through Light and Time
2024年10月5日 · NGC 428 is a distorted spiral galaxy located approximately 54 million light years away in the constellation Cetus. It is classified as SAB (s)m with HII emission. It has been observed that there are two bar-like bright regions indicating that an interaction may be occurring or may have occurred with another galaxy. Possibly PGC 135629.
H I and optical observations of the NGC 428 field. - NASA/ADS
The H I and optical properties of the NGC 428 galaxy field are presented. Three galaxies in this system are found to contain H I. The largest of these is NGC 428 which has undergone strong recent star formation in its spiral arms where the H I surface density exceeds ≈8×10<SUP>20</SUP>cm<SUP>-2</SUP>.
NGC 428 Facts (UGC 763) & Distance - Universe Guide
NGC 428 is an Active Galactic Nuclei/Nucleus located in the constellation of Cetus in the equatorial region. NGC 428's distance from Earth is 40,710,839.06 light years. NGC 428 is called NGC 428 in the New General Catalogue (NGC).