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ngc_4150_elliptical_hst.jpeg | Kavli Institute for Cosmology,…
https://www.kicc.cam.ac.uk/file/ngc4150ellipticalhstjpeg27 Mar 2024: Search site. Kavli Institute for Cosmology, Cambridge. ngc_4150_elliptical_hst.jpeg. Alt Text:. An image of the quiescent elliptical galaxy NGC 4150, made with the Hubble Space Telescope. -
Recent IoA Publications | Institute of Astronomy
https://www.ast.cam.ac.uk/aggregator/sources/2227 Mar 2024: Uncovering the Ghostly Remains of an Extremely Diffuse Satellite in the Remote Halo of NGC,253. ... We conclude that the broad-line region in NGC 1566 is dominated by the kinematics of a relativistic eccentric accretion disk. -
Feed aggregator | Institute of Astronomy
https://www.ast.cam.ac.uk/aggregator27 Mar 2024: the Sculptor Group spiral, NGC 253. ... The distribution of red giant branch stars is asymmetrical and displays two elongated tidal extensions pointing towards NGC 253, suggestive of a highly disrupted system being observed at apocenter. -
Lists of good telescope targets | Institute of Astronomy - Public
https://www.public.ast.cam.ac.uk/lists-good-telescope-targets27 Mar 2024: NGC 869/884 (Perseus double cluster). Both clusters lie in a nearby spiral arm of our galaxy. ... NGC 663 in Cass. Mag 7. 400 stars in a scattered open cluster 8000ly distant. -
Prof. Kaisey Mandel | Institute of Astronomy
https://www.ast.cam.ac.uk/people/kaisey.mandel27 Mar 2024: et al. (The Young Supernova Experiment). 2023. Relative intrinsic scatter in hierarchical Type Ia supernova siblings analyses: Application to SNe 2021hpr, 1997bq & 2008fv in NGC 3147. -
https://www.ast.cam.ac.uk/news/feed
https://www.ast.cam.ac.uk/news/feed27 Mar 2024: artists-impression-of-the-surroundings-of-the-supermassive-black-hole-in-ngc-3783-dp.jpg?itok=bw3WOEUy" alt="" /></a></div></div></div><div class="field field-name-body -
https://www.ast.cam.ac.uk/aggregator/rss
https://www.ast.cam.ac.uk/aggregator/rss27 Mar 2024: Tue, 26 Mar 2024 10:13:00 0000 Recent IoA Publications: Uncovering the Ghostly Remains of an Extremely Diffuse Satellite in the Remote Halo of NGC,253 ... The distribution of red giant branch stars is asymmetrical and displays two elongated tidal -
Julia Sisk-Reynes | Institute of Astronomy
https://www.ast.cam.ac.uk/people/Julia.Sisk-Reynes27 Mar 2024: An X-ray Case Study with NGC 1275 - James H. Matthews, Christopher S. -
Neon sign identified by JWST gives clue to planet formation |…
https://www.ast.cam.ac.uk/news/neon-sign-identified-jwst-gives-clue-planet-formation27 Mar 2024: Search site. Institute of Astronomy. Neon sign identified by JWST gives clue to planet formation. Submitted by Matthew Bothwell on Tue, 05/03/2024 - 15:31. The winds that help to form planets in the gaseous discs of early solar systems have been -
The Murdin Prize | Institute of Astronomy
https://www.ast.cam.ac.uk/current-students/postgraduate/your-phd/murdin-prize27 Mar 2024: Peter Kosec - Evidence for a Variable Ultrafast Outflow in the Newly Discovered Ultraluminous Pulsar NGC 300 ULX-1.
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