2,340 research outputs found
Local scale invariance in the parity conserving nonequilibrium kinetic Ising model
The local scale invariance has been investigated in the nonequilibrium
kinetic Ising model exhibiting absorbing phase transition of PC type in 1+1
dimension. Numerical evidence has been found for the satisfaction of this
symmetry and estimates for the critical ageing exponents are given.Comment: 8 pages, 2 figures (IOP format), final form to appear in JSTA
The detection of extragalactic N: Consequences for nitrogen nucleosynthesis and chemical evolution
Detections of extragalactic N are reported from observations of the
rare hydrogen cyanide isotope HCN toward the Large Magellanic Cloud
(LMC) and the core of the (post-) starburst galaxy NGC 4945. Accounting for
optical depth effects, the LMC data from the massive star-forming region N113
infer a N ratio of 111 17, about twice the C
value. For the LMC star-forming region N159HW and for the central region of NGC
4945, N ratios are also 100. The N ratios
are smaller than all interstellar nitrogen isotope ratios measured in the disk
and center of the Milky Way, strongly supporting the idea that N is
predominantly of `primary' nature, with massive stars being its dominant
source. Although this appears to be in contradiction with standard stellar
evolution and nucleosynthesis calculations, it supports recent findings of
abundant N production due to rotationally induced mixing of protons into
the helium-burning shells of massive stars.Comment: 15 pages including one postscript figure, accepted for publication by
ApJ Letter, further comments: please contact Yi-nan Chi
On the universality of luminosity-metallicity and mass-metallicity relations for compact star-forming galaxies at redshifts 0 < z < 3
We study relations between global characteristics of low-redshift (0 < z < 1)
compact star-forming galaxies, including absolute optical magnitudes, Hbeta
emission-line luminosities (or equivalently star-formation rates), stellar
masses, and oxygen abundances. The sample consists of 5182 galaxies with
high-excitation HII regions selected from the SDSS DR7 and SDSS/BOSS DR10
surveys adopting a criterion [OIII]4959/Hbeta > 1. These data were combined
with the corresponding data for high-redshift (2 < z < 3) star-forming
galaxies. We find that in all diagrams low-z and high-z star-forming galaxies
are closely related indicating a very weak dependence of metallicity on stellar
mass, redshift, and star-formation rate. This finding argues in favour of the
universal character of the global relations for compact star-forming galaxies
with high-excitation HII regions over redshifts 0 < z < 3.Comment: 13 pages, 10 figures, accepted for publication in MNRA
Searching for metal-deficient emission-line galaxy candidates: the final sample of the SDSS DR12 galaxies
We present a spectroscopic study of metal-deficient dwarf galaxy candidates,
selected from the SDSS DR12. The oxygen abundances were derived using the
direct method in galaxies with the electron temperature-sensitive emission line
[OIII]4363A measured with an accuracy better than 30%. The oxygen abundances
for the remaining galaxies with larger uncertainties of the [OIII]4363A line
fluxes were calculated using a strong-line semi-empirical method by Izotov and
Thuan. The resulting sample consists of 287 low-metallicity candidates with
oxygen abundances below 12+logO/H=7.65 including 23 extremely metal-deficient
(XMD) candidates with 12+log O/H<7.35. Ten out of sixteen XMDs known so far (or
~60%) have been discovered by our team using the direct method. Three XMDs were
found in the present study. We study relations between global parameters of
low-metallicity galaxies, including absolute optical magnitudes, Hbeta
luminosities (or equivalently star formation rates), stellar masses,
mid-infrared colours, and oxygen abundances. Low-metallicity and XMD galaxies
strongly deviate to lower metallicities in L-Z, L(Hbeta)-Z and Mstar-Z diagrams
than in relations obtained for large samples of low-redshift, star-forming
galaxies with non-restricted metallicities. These less chemically evolved
galaxies with stellar masses ~10^6-10^8Msun, Hbeta luminosities ~10^38-10^41
erg/s, SFR~0.01-1.0Msun/yr, and sSFR~50 Gyr^-1 have physical conditions which
may be characteristic of high-redshift low-mass star-forming galaxies which are
still awaiting discovery.Comment: 13 pages, 6 figures, accepted for publication in Astronomy and
Astrophysic
New candidates for extremely metal-poor emission-line galaxies in the SDSS/BOSS DR10
We present a spectroscopic study of eight extremely low-metallicity candidate
emission-line galaxies with oxygen abundances possibly below 12 +log O/H =
7.35. These galaxies were selected from Data Release 10 of the Sloan Digital
Sky Survey/Baryon Oscillation Spectroscopic Survey (SDSS/BOSS DR10). We will
call these extremely metal-deficient galaxies XMD galaxies. The electron
temperature-sensitive emission line [O~{\sc iii}] 4363 is detected in
three galaxies and marginally detected in two galaxies, allowing for abundance
determination by a "direct" method. Because of large uncertainties in the [O
{\sc iii}]4363\AA\ line fluxes, we also calculated oxygen abundance in
these galaxies together with the remaining three galaxies using a strong-line
semi-empirical method. This method gives oxygen abundances higher than 7.35 for
three galaxies with detected [O {\sc iii}]4363\AA\ line and lower than
7.35 for the remaining five objects of the sample. The newly-discovered
galaxies represent excellent targets for follow-up spectroscopic observations
with the largest telescopes to improve the oxygen abundance determination and
to increase the number of these very rare low-metallicity objects. The extreme
location of the most massive and luminous XMD galaxies and XMD candidates in
the stellar mass-metallicity diagram implies that these galaxies may be genuine
young objects.
With stellar masses of up to 10 - 10, the galaxies
are not chemically enriched and strongly deviate to lower metallicity as
compared to the relation obtained for a large sample of low-redshift,
star-forming galaxies.Comment: 10 pages, 5 figures, 4 tables, accepted in Astronomy and Astrophysic
The Mg II 2797, 2803 emission in low-metallicity star-forming galaxies from the SDSS
We present 65 Sloan Digital Sky Survey (SDSS) spectra of 62 star-forming
galaxies with oxygen abundances 12 + logO/H ~ 7.5-8.4. Redshifts of selected
galaxies are in the range z~0.36-0.70. This allows us to detect the redshifted
MgII 2797,2803 emission lines. Our aim is to use these lines for the magnesium
abundance determination. The MgII emission was detected in ~2/3 of the
galaxies. We find that the MgII 2797 emission-line intensity follows a trend
with the excitation parameter x= O^{2+}/O that is similar to that predicted by
CLOUDY photoionised HII region models, suggesting a nebular origin of MgII
emission. The Mg/O abundance ratio is lower by a factor ~2 than the solar
ratio. This is probably the combined effect of interstellar MgII absorption and
depletion of Mg onto dust. However, the effect of dust depletion in selected
galaxies, if present, is small, by a factor of ~2 lower than that of iron.Comment: Accepted for publication in Astronomy and Astrophysics, 14 pages, 8
figure
VLT/X-shooter observations of blue compact galaxies Haro 11 and ESO 338-IG 004
(abridged) Strongly star-forming galaxies of subsolar metallicities are
typical of the high-redshift universe. Here we therefore provide accurate data
for two low-z analogs, the well-known low-metallicity emission-line galaxies
Haro 11 and ESO 338-IG 004. On the basis of Very Large Telescope/X-shooter
spectroscopic observations in the wavelength range 3000-24000\AA, we use
standard direct methods to derive physical conditions and element abundances.
Furthermore, we use X-shooter data together with Spitzer observations in the
mid-infrared range to attempt to find hidden star formation. We derive
interstellar oxygen abundances of 12 + log O/H = 8.33+/-0.01, 8.10+/-0.04, and
7.89+/-0.01 in the two HII regions B and C of Haro 11 and in ESO 338-IG 004,
respectively. The observed fluxes of the hydrogen lines correspond to the
theoretical recombination values after correction for extinction with a single
value of the extinction coefficient C(Hbeta) across the entire wavelength range
from the near-ultraviolet to the NIR and mid-infrared for each of the studied
HII regions. Therefore there are no emission-line regions contributing to the
line emission in the NIR range, which are hidden in the optical range. The
agreement between the extinction-corrected and CLOUDY-predicted fluxes implies
that a HII region model including only stellar photoionisation is able to
account for the observed fluxes, in both the optical and NIR ranges. All
observed spectral energy distributions (SEDs) can be reproduced quite well
across the whole wavelength range by model SEDs except for Haro 11B, where
there is a continuum flux excess at wavelengths >1.6mum. It is possible that
one or more red supergiant stars are responsible for the NIR flux excess in
Haro 11B. We find evidence of a luminous blue variable (LBV) star in Haro 11C.Comment: 18 pages, 6 figures. Accepted for publication in Astronomy and
Astrophysic
Connecting the Micro-dynamics to the Emergent Macro-variables: Self-Organized Criticality and Absorbing Phase Transitions in the Deterministic Lattice Gas
We reinvestigate the Deterministic Lattice Gas introduced as a paradigmatic
model of the 1/f spectra (Phys. Rev. Lett. V26, 3103 (1990)) arising according
to the Self-Organized Criticality scenario. We demonstrate that the density
fluctuations exhibit an unexpected dependence on systems size and relate the
finding to effective Langevin equations. The low density behavior is controlled
by the critical properties of the gas at the absorbing state phase transition.
We also show that the Deterministic Lattice Gas is in the Manna universality
class of absorbing state phase transitions. This is in contrast to expectations
in the literature which suggested that the entirely deterministic nature of the
dynamics would put the model in a different universality class. To our
knowledge this is the first fully deterministic member of the Manna
universality class.Comment: 8 pages, 12 figures. Changes in the new version: Reference list has
been correcte
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