Journal article icon

Journal article

Supermassive black hole mass measurements for NGC 1300 and NGC 2748 based on HST emission-line gas kinematics

Abstract:
We present Space Telescope Imaging Spectrograph emission-line spectra of the central regions of the spiral galaxies NGC 1300 and NGC 2748. From the derived kinematics of the nuclear gas we have found evidence for central supermassive black holes in both galaxies. The estimated mass of the black hole in NGC 1300 is 6.6 (+6.3, -3.2) x 10^7 solar masses and in NGC 2748 is 4.4 (+3.5, -3.6) x 10^7 solar masses (both at the 95% confidence level). These two black hole mass estimates contribute to the poorly sampled low-mass end of the nuclear black hole mass spectrum.
Publication status:
Published

Actions


Access Document


Publisher copy:
10.1111/j.1365-2966.2005.08904.x

Authors



Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
359
Issue:
2
Pages:
504-520
Publication date:
2005-02-28
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
pubs:19269
UUID:
uuid:bdf78728-aa12-43ef-944e-2a9ddf38edab
Local pid:
pubs:19269
Source identifiers:
19269
Deposit date:
2012-12-19

Terms of use



Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP