SwePub
Sök i LIBRIS databas

  Extended search

WFRF:(Forman W.)
 

Search: WFRF:(Forman W.) > The ALMA Discovery ...

The ALMA Discovery of the Rotating Disk and Fast Outflow of Cold Molecular Gas in NGC 1275

Nagai, H. (author)
National Astronomical Observatory of Japan,The Graduate University for Advanced Studies (SOKENDAI)
Onishi, Kyoko, 1989 (author)
Chalmers tekniska högskola,Chalmers University of Technology,Ehime University
Kawakatu, N. (author)
National Institute of Technology, Kure College
show more...
Fujita, Y. (author)
Osaka University
Kino, M. (author)
National Astronomical Observatory of Japan,Kogakuin University of Technology and Engineering
Fukazawa, Y. (author)
Hiroshima University
Lim, J. (author)
The University of Hong Kong
Forman, W. (author)
Harvard-Smithsonian Center for Astrophysics
Vrtilek, J. (author)
Harvard-Smithsonian Center for Astrophysics
Nakanishi, K. (author)
The Graduate University for Advanced Studies (SOKENDAI),National Astronomical Observatory of Japan
Noda, H. (author)
Osaka University
Asada, K. (author)
Academia Sinica Taiwan
Wajima, K. (author)
Korea Astronomy and Space Science Institute
Ohyama, Y. (author)
Academia Sinica Taiwan
David, L. (author)
Harvard-Smithsonian Center for Astrophysics
Daikuhara, K. (author)
Toho University
show less...
 (creator_code:org_t)
2019-10-04
2019
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 883:2
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We present observations using the Atacama Large Millimeter/submillimeter Array of the CO(2-1), HCN(3-2), and HCO+(3-2) lines in the nearby radio galaxy/brightest cluster galaxy (BCG) NGC 1275 with a spatial resolution of similar to 20 pc. In previous observations, the CO(2-1) emission was detected as radial filaments lying in the east west direction on a kiloparsec scale. We resolved the inner filament and found that it cannot be represented by a simple infalling stream on a sub-kiloparsec scale. The observed complex nature of the filament resembles the cold gas structure predicted by numerical simulations of cold chaotic accretion. Within the central 100 pc, we detected a rotational disk of molecular gas whose mass is similar to 10(8) M-circle dot. This is the first evidence of the presence of a massive cold gas disk on this spatial scale for BCGs. A crude estimate suggests that the accretion rate of the cold gas can be higher than that of hot gas. The disk rotation axis is approximately consistent with the radio-jet axis. This probably suggests that the cold gas disk is physically connected to the innermost accretion disk, which is responsible for jet launching. We also detected absorption features in the HCN(3-2) and HCO+(3-2) spectra against the radio continuum emission mostly radiated by a jet of size similar to 1.2 pc. The absorption features are blueshifted from the systemic velocity by similar to 300-600 km s(-1), suggesting the presence of outflowing gas from the active galactic nucleus (AGN). We discuss the relation of the AGN feeding with cold accretion, the origin of blueshifted absorption, and an estimate of the black hole mass using molecular gas dynamics.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

galaxies: active
galaxies: elliptical and lenticular, cD
galaxies: individual (3C 84, NGC 1275, Perseus A)
galaxies: nuclei

Publication and Content Type

art (subject category)
ref (subject category)

Find in a library

To the university's database

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view