
Using the James Webb Space Telescope (JWST), an international team of astronomers has observed an elliptical galaxy known as NGC 4486B. Results of the observational campaign, published Dec. 16 on the arXiv preprint server, deliver important insights into the properties of the double nucleus of this galaxy.
Why does NGC 4486B have a double nucleus?
NGC 4486B (also known as VCC1279) is a compact elliptical galaxy at the center of the Virgo Cluster. It has a small effective radius of about 620 light years, an absolute magnitude of 17.6 mag, and its total stellar mass is estimated to be approximately 6 billion solar masses.
Hubble Space Telescope observations of NGC 4486B have revealed that it hosts a double nucleus, as does the Andromeda galaxy...
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