Continuing formation of the central star cluster in M87
- 1 January 1984
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 307 (5949) , 343
- https://doi.org/10.1038/307343a0
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Further evidence for M87's massive, dark haloThe Astrophysical Journal, 1983
- Star formation in a cooling flowMonthly Notices of the Royal Astronomical Society, 1982
- X-ray spectroscopy of the galaxy M87 - Radiative accretion of the hot plasma haloThe Astrophysical Journal, 1982
- Einstein Observatory solid state spectrometer observations of M87 and the Virgo clusterThe Astrophysical Journal, 1982
- The Spectrum of the Central Luminosity Spike in M87The Astrophysical Journal, 1980
- High-resolution X-ray spectroscopy of M87 with the Einstein observatory - The detection of an O VIII emission lineThe Astrophysical Journal, 1979
- Luminosity distribution in the central regions of Messier 87 - Isothermal core, point source, or black holeThe Astrophysical Journal, 1979
- Dynamical evidence for a central mass concentration in the galaxy M87The Astrophysical Journal, 1978
- Evidence for a supermassive object in the nucleus of the galaxy M87 from SIT and CCD area photometryThe Astrophysical Journal, 1978
- Subsonic accretion of cooling gas in clusters of galaxiesMonthly Notices of the Royal Astronomical Society, 1977