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Interferometric Mapping of Magnetic fields: The Alma view of the Massive star-forming clump W43-MM1
(IOP, 2016)
Here, we present the first results from ALMA observations of 1 mm polarized dust emission toward the W43-MM1 high-mass star-forming clump. We have detected a highly fragmented filament with source masses ranging from 14 ...
Interferometric mapping of magnetic fields: The massive star-forming region G34.4+0.23 MM
(UNIV CHICAGO PRESS, 2008-03-20)
We report millimeter interferometric observations of polarized continuum and line emission from the massive star-forming region G34.4. Polarized thermal dust emission at 3 mm wavelength and CO J = 1 -> 0 line emission were ...
A MINI element over star convex polytopes
(Elsevier, 2020)
In this paper, we extend the concept of MINI element over triangles to star convex arbitrary polytopes. This is achieved by employing the volume averaged nodal projection (VANP) method over polytopes in combination with ...
Estimation of exoplanetary planet-to-star radius ratio with homomorphic processing
(Elsevier, 2017)
In this paper a homomorphic filtering scheme is proposed to improve the estimation of the planet/star
radius ratio in astronomical transit signals. The idea is to reduce the effect of the short-term earth
atmosphere ...
Extreme star formation in the host galaxies of the fastest growing supermassive black holes AT z = 4.8
(2012-04-20)
We report new Herschel observations of 25 z 4.8 extremely luminous optically selected active galactic nuclei
(AGNs). Five of the sources have extremely large star-forming (SF) luminosities, LSF, corresponding to SF ...
Magnetic field evolution in neutron stars: one-dimensional multi-fluid model
(EDP SCIENCES S A, 2008-09)
Aims. This paper is the first in a series that aims to understand the long-term evolution of neutron star magnetic fields.
Methods. We model the stellar matter as an electrically neutral and lightly-ionized plasma composed ...
SIMBA survey of southern high-mass star forming regions - I. Physical parameters of the 1.2-mm/IRAS sources
(E D P SCIENCES, 2004-10)
We report the results of a 1.2 mm continuum emission survey toward 146 IRAS sources thought to harbour high-mass star forming regions. The sources have FIR colors typical of UCHII regions and were detected in the CS(2 --> ...
Separate ways: the mass-metallicity relation does not strongly correlate with star formation rate in SDSS-IV MaNGA galaxies
(IOP Publishing Ltd, 2017)
We present the integrated stellar mass-metallicity relation (MZR) for more than 1700 galaxies included in the integral field area SDSS-IV MaNGA survey. The spatially resolved data allow us to determine the metallicity at ...
Differential form of the star product for SU(2) Stratonovich-Weyl symbols
(2003)
An exact differential form for the star product is derived and its asymptotic form in the limit of large spin is analyzed. As an immediate application we obtain evolution equations for a class of s-parametrized SU(2) ...
Differential form of the star product for SU(2) Stratonovich-Weyl symbols
(2003)
An exact differential form for the star product is derived and its asymptotic form in the limit of large spin is analyzed. As an immediate application we obtain evolution equations for a class of s-parametrized SU(2) ...