SwePub
Sök i LIBRIS databas

  Extended search

WFRF:(Kawamuro Taiki)
 

Search: WFRF:(Kawamuro Taiki) > (2020) > AGN X-Ray Irradiati...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

AGN X-Ray Irradiation of CO Gas in NGC 2110 Revealed by Chandra and ALMA

Kawamuro, Taiki (author)
National Astronomical Observatory of Japan
Izumi, Takuma (author)
National Astronomical Observatory of Japan,The Graduate University for Advanced Studies (SOKENDAI)
Onishi, Kyoko, 1989 (author)
Chalmers tekniska högskola,Chalmers University of Technology
show more...
Imanishi, Masatoshi (author)
National Astronomical Observatory of Japan,The Graduate University for Advanced Studies (SOKENDAI)
Nguyen, Dieu D. (author)
National Astronomical Observatory of Japan
Baba, Shunsuke (author)
National Astronomical Observatory of Japan
show less...
 (creator_code:org_t)
2020-06-04
2020
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 895:2
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We report spatial distributions of the Fe-K alpha line at 6.4 keV and the CO(J = 2-1) line at 230.538 GHz in NGC 2110, which are, respectively, revealed by Chandra and Atacama Large Millimeter/submillimeter Array (ALMA) at 05. A Chandra 6.2-6.5 keV to 3.0-6.0 keV image suggests that the Fe-K alpha emission extends preferentially in a northwest to southeast direction out to 3 '', or similar to 500 pc, on each side. Spatially resolved spectral analyses support this by finding significant Fe-K alpha emission lines only in the northwest and southeast regions. Moreover, their equivalent widths are found to be similar to 1.5 keV, indicative for the fluorescence by nuclear X-ray irradiation as the physical origin. By contrast, CO(J = 2-1) emission is weak therein. For quantitative discussion, we derive ionization parameters by following an X-ray dominated region (XDR) model. We then find them high enough to interpret the weakness as the result of X-ray dissociation of CO and/or H-2. Another possibility also remains that CO molecules follow a superthermal distribution, resulting in brighter emission in higher-J lines. Further follow-up observations are encouraged to draw a conclusion on what predominantly changes the interstellar matter properties and whether the X-ray irradiation eventually affects the surrounding star formation as active galactic nucleus (AGN) feedback.

Subject headings

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

Keyword

Molecular gas
AGN host galaxies
Star formation
X-ray active galactic nuclei
Radio astronomy
Submillimeter astronomy
X-ray astronomy
Astrophysical black holes
Active galactic nuclei

Publication and Content Type

art (subject category)
ref (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Search outside SwePub

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