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- W2063761284 abstract "view Abstract Citations (48) References (16) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The infrared source near the rapid-burst X-ray source MXB 1730-335. Kleinmann, D. E. ; Kleinmann, S. G. ; Wright, E. L. Abstract Photometry at 1-5 microns shows that the faint optical source inferred to be a globular cluster associated with MXB 1730-335 is indeed one of the most highly concentrated globular clusters known, with a core diameter of 13 plus or minus 1 sec (0.6 pc at 10 kpc). Its central surface brightness is 0.6 mag brighter than the next brightest globular cluster, NGC 6440, which is also associated with an X-ray source. The surface brightness and core radius of the globular cluster associated with MXB 1730-335 indicate a central density of 4 x 10 to the 5th solar masses/cu pc, a central escape velocity of 60 km/s, and a relaxation time of 4 x 10 to the 7th years. Publication: The Astrophysical Journal Pub Date: December 1976 DOI: 10.1086/182309 Bibcode: 1976ApJ...210L..83K Keywords: Astronomical Photometry; Globular Clusters; Infrared Astronomy; Radiant Flux Density; X Ray Sources; Brightness; Spectral Energy Distribution; Astrophysics full text sources ADS | data products SIMBAD (3)" @default.
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- W2063761284 date "1976-12-01" @default.
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- W2063761284 title "The infrared source near the rapid-burst X-ray source MXB 1730-335" @default.
- W2063761284 doi "https://doi.org/10.1086/182309" @default.
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