Disentangling the Circumnuclear Environs of Centaurus A. II. On the Nature of the Broad Absorption Line
Artikel i vetenskaplig tidskrift, 2010
We report on atomic gas (H I) and molecular gas (as traced by CO(2-1)) redshifted absorption features toward the nuclear regions of the closest powerful radio galaxy, Centaurus A (NGC 5128). Our H I observations using the Very Long Baseline Array allow us to discern with unprecedented sub-parsec resolution H I absorption profiles toward different positions along the 21 cm continuum jet in the inner 0farcs3 (or 5.4 pc). In addition, our CO(2-1) data obtained with the Submillimeter Array probe the bulk of the absorbing molecular gas with little contamination by emission, which was not possible with previous CO single-dish observations. We shed light on the physical properties of the gas in the line of sight with these data, emphasizing the still open debate about the nature of the gas that produces the broad absorption line (~55 km s–1). First, the broad H I line is more prominent toward the central and brightest 21 cm continuum component than toward a region along the jet at a distance ~20 mas (or 0.4 pc) further from the nucleus. This indicates that the broad absorption line arises from gas located close to the nucleus, rather than from diffuse and more distant gas. Second, the different velocity components detected in the CO(2-1) absorption spectrum match well with other molecular lines, such as those of HCO+(1-0), except the broad absorption line that is detected in HCO+(1-0) (and most likely related to that of the H I). Dissociation of molecular hydrogen due to the active galactic nucleus seems to be efficient at distances r lsim 10 pc, which might contribute to the depth of the broad H I and molecular lines.
quasars: absorption lines
cD
galaxies: elliptical and lenticular
galaxies: ISM
galaxies: individual (NGC 5128)
galaxies: structure
Författare
D. Espada
Harvard-Smithsonian Center for Astrophysics
Academia Sinica
Consejo Superior de Investigaciones Científicas (CSIC)
A. B. Peck
National Radio Astronomy Observatory Socorro
Harvard-Smithsonian Center for Astrophysics
Atacama Large Millimeter-submillimeter Array (ALMA)
S. Matsushita
Academia Sinica
Atacama Large Millimeter-submillimeter Array (ALMA)
K. Sakamoto
Academia Sinica
C. Henkel
Max-Planck-Gesellschaft
D. Iono
National Astronomical Observatory of Japan
F. P. Israel
Universiteit Leiden
Sebastien Muller
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
G. Petitpas
Harvard-Smithsonian Center for Astrophysics
Y. Pihlstrom
National Radio Astronomy Observatory Socorro
University of New Mexico
G. Taylor
National Radio Astronomy Observatory Socorro
University of New Mexico
D.-V. Trung
Academia Sinica
Vietnam Academy of Science and Technology
Publicerad i
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 720 Nummer/häfte 1 s. 666-678Kategorisering
Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
Identifikatorer
DOI
10.1088/0004-637X/720/1/666