470 research outputs found
The Spectral Energy Distribution of Normal, Starburst and Active Galaxies
We present the results of an extensive literature search of multiwavelength
data for a sample of 59 galaxies, consisting of 26 Starbursts, 15 Seyfert 2's,
5 LINER's, 6 normal spirals and 7 normal elliptical galaxies. The data include
soft X-ray fluxes, ultraviolet and optical spectra, near, mid/far infrared
photometry and radio measurements, selected to match as closely as possible the
IUE aperture (10" X 20"). The galaxies are separated into 6 groups with similar
characteristics, namely, Ellipticals, Spirals, LINER's, Seyfert 2's, Starbursts
of Low and High reddening, for which we create average spectral energy
distributions (SED). The individual groups SED's are normalized to the
7000\AA flux and compared, looking for similarities and differences
among them.The bolometric fluxes of different types of galaxies were calculated
integrating their SED's. These values are compared with individual waveband
flux densities, in order to determine the wavebands which contribute most to
the bolometric flux. Linear regressions were performed between the bolometric
and individual band fluxes for each kind of galaxy. These fits can be used in
the calculation of the bolometric flux for other objects of similar activity
type, but with reduced waveband information. We have also collected
multiwavelength data for 4 HII regions, a thermal supernova remnant, and a
non-thermal supernova remnant (SNR), which are compared with the Starburst
SED's.Comment: 29 pages, 13 postscript figures and 10 tables. To appear in The
Astronomical Journa
Transition (LINER/HII) nuclei as evolved Composite (Seyfert 2/Starburst) nuclei
We compare the circumnuclear stellar population and environmental properies
of Seyfert and Composite (Seyfert + Starburst) nuclei with those of LINERs and
LINER/HII transition galaxies (TOs), and discuss evidences for evolution from
Seyfert/Composite to LINER/TO nuclei.Comment: 2 pages, 1 figure; to appear in the Proceedings of IAU Symp. No. 222:
The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, CUP, eds.
T. Storchi-Bergmann, L. Ho and H. R. Schmit
The Ionizing Source of the Nucleus of NGC1097
We present new observations in X-ray and optical/ultraviolet of the nucleus
of NGC1097, known for the abrupt appearance of broad, double-peaked Balmer
lines in its spectrum in 1991. These new observations are used to construct the
spectral energy distribution (SED) of the central engine. From the SED we infer
that this AGN is radio-loud and has a bolometric luminosity L_Bol ~ 10^42
erg/s, implying a low Eddington ratio of L_Bol/L_Edd ~ 10^{-4}. These results
suggest that the central ionizing source is an advection-dominated accretion
flow (ADAF) in the form of an ellevated structure which photoionizes an outer
thin disk. We fit a simplified ADAF model to the SED and obtain limits on the
values of the mass accretion rate Mdot and accretion efficiency \eta, namely
Mdot/Mdot_Edd >= 10^{-3} and \eta <= 10^{-2}. We identify an energy budget
problem: if the central photoionizing source is isotropic, the covering factor
of the line-emitting portion of the thin accretion disk is ~ 6, i. e. the
central source accounts for only 20% of the energy emitted in the double-peaked
Balmer lines.Comment: 4 pages, 3 figures, to appear in the proceedings of "The Interplay
among Black Holes, Stars and ISM in Galactic Nuclei", IAU 222, eds. Th.
Storchi Bergmann, L.C. Ho, and H.R. Schmit
2D mapping of young stars in the inner 180 pc of NGC 1068: correlation with molecular gas ring and stellar kinematics
We report the first two-dimensional mapping of the stellar population and
non-stellar continua within the inner 180 pc (radius) of NGC 1068 at a spatial
resolution of 8 pc, using integral field spectroscopy in the near-infrared. We
have applied the technique of spectral synthesis to data obtained with the
instrument NIFS and the adaptive optics module ALTAIR at the Gemini North
Telescope. Two episodes of recent star formation are found to dominate the
stellar population contribution: the first occurred 300 Myr ago, extending over
most of the nuclear region; the second occurred just 30 Myr ago, in a ring-like
structure at ~100 pc from the nucleus, where it is coincident with an expanding
ring of H2 emission. Inside the ring, where a decrease in the stellar velocity
dispersion is observed, the stellar population is dominated by the 300 Myr age
component. In the inner 35 pc, the oldest age component (age > 2Gyr) dominates
the mass, while the flux is dominated by black-body components with
temperatures in the range 700 < T < 800 K which we attribute to the dusty
torus. We also find some contribution from black-body and power-law components
beyond the nucleus which we attribute to dust emission and scattered light.Comment: Accepted for publication in Ap
A New Superwind Wolf-Rayet Galaxy Mrk 1259
We report the discovery of a starburst-driven wind (superwind) from the
starburst nucleus galaxy Mrk 1259. The estimated number ratio of Wolf-Rayet
(WR) to O stars amounts to ~0.09. While the nuclear emission-line region is due
to usual photoionization by massive stars, the circumnuclear emission-line
regions show anomalous line ratios that can be due to cooling shocks. Since the
host galaxy seems to be a face-on disk galaxy and the excitation conditions of
the circumnuclear emission-line regions show the spatial symmetry, we consider
that we are seeing the superwind nearly from a pole-on view. Cooling shock
models may explain the observed emission line ratios of the circumnuclear
regions although a factor of 2 overabundance of nitrogen is necessary. All
these suggest that the high-mass enhanced starburst occurred ~5X10^6 years ago
in the nuclear region of Mrk 1259.Comment: To be published in the Astrophysical Journal Letters, 15 pages, 4
figure
On the nature of the near-UV extended light in Seyfert galaxies
We study the nature of the extended near-UV emission in the inner kiloparsec
of a sample of 15 Seyfert galaxies which have both near-UV (F330W) and narrow
band [OIII] high resolution Hubble images. For the majority of the objects we
find a very similar morphology in both bands. From the [OIII] images we
construct synthetic images of the nebular continuum plus the emission line
contribution expected through the F330W filter, which can be subtracted from
the F330W images. We find that the emission of the ionised gas dominates the
near-UV extended emission in half of the objects. A further broad band
photometric study, in the bands F330W (U), F547M (V) and F160W (H), shows that
the remaining emission is dominated by the underlying galactic bulge
contribution. We also find a blue component whose nature is not clear in 4 out
of 15 objects. This component may be attributed to scattered light from the
AGN, to a young stellar population in unresolved star clusters, or to
early-disrupted clusters. Star forming regions and/or bright off-nuclear star
clusters are observed in 4/15 galaxies of the sample.Comment: 23 pages, 6 figures, 3 tables; accepted for publication in MNRA
An atlas of Calcium triplet spectra of active galaxies
We present a spectroscopic atlas of active galactic nuclei covering the
region around the 8498, 8542, 8662 Calcium triplet (CaT) lines. The sample
comprises 78 objects, divided into 43 Seyfert 2s, 26 Seyfert 1s, 3 Starburst
and 6 normal galaxies. The spectra pertain to the inner ~300 pc in radius, and
thus sample the central kinematics and stellar populations of active galaxies.
The data are used to measure stellar velocity dispersions (sigma_star) both
with cross-correlation and direct fitting methods. These measurements are found
to be in good agreement with each-other and with those in previous studies for
objects in common. The CaT equivalent width is also measured. We find average
values and sample dispersions of W_CaT of 4.6+/-2.0, 7.0 and 7.7+/-1.0
angstrons for Seyfert 1s, Seyfert 2s and normal galaxies, respectively. We
further present an atlas of [SIII]\lambda 9069 emission line profiles for a
subset of 40 galaxies. These data are analyzed in a companion paper which
addresses the connection between stellar and Narrow Line Region kinematics, the
behaviour of the CaT equivalent width as a function of sigma_star, activity
type and stellar population properties.Comment: 18 pages, 10 figures, accepted for publication in MNRA
- …