9.13. Story of the discovery of a massive black hole in NGC4258
1998 ◽
Vol 184
◽
pp. 407-408
In the Autumn of 1991, Nakai et al.(1993) began monitoring observations of water mega masers including NGC4258 using Nobeyama 45 m telescope. The 45 m telescope was equipped with wide band cooled HEMT receiver (22 GHz) and wide band spectrometers (AOS). Nakai used 8 AOSs which covered 4480 km/sec in velocity. It was from the wide-band system that the high velocity maser components were detected unexpectedly which locate ±1000 km/sec from the known features of the NGC4258 (Claussen et al. 1984). The finding was in May 1992 when busy Nakai got time checking the data deeply, half year had passed since the beginning of the observations.
2002 ◽
Vol 206
◽
pp. 400-403
Keyword(s):
2016 ◽
Vol 458
(3)
◽
pp. 2596-2603
◽
2013 ◽
Vol 9
(S298)
◽
pp. 421-421
Keyword(s):
2009 ◽
Vol 692
(2)
◽
pp. 1075-1109
◽
Keyword(s):
Effects of supernovae feedback and black hole outflows in the evolution of Dwarf Spheroidal Galaxies
2020 ◽
Vol 15
(S359)
◽
pp. 280-282
Keyword(s):
2019 ◽
Vol 15
(S359)
◽
pp. 312-317
Keyword(s):
Keyword(s):