1,031 research outputs found
BhaBAR: Big Halpha kinematical sample of BARred spiral galaxies - I. Fabry-Perot Observations of 21 galaxies
The Halpha gas kinematics of twenty-one representative barred spiral galaxies
belonging to the BHaBAR sample is presented. The galaxies were observed with
FaNTOmM, a Fabry-Perot integral-field spectrometer, on three different
telescopes. The 3D data cubes were processed through a robust pipeline with the
aim of providing the most homogeneous and accurate dataset possible useful for
further analysis. The data cubes were spatially binned to a constant
signal-to-noise ratio, typically around 7. Maps of the monochromatic Halpha
emission line and of the velocity field were generated and the kinematical
parameters were derived for the whole sample using tilted-ring models. The
photometrical and kinematical parameters (position angle of the major axis,
inclination, systemic velocity and kinematical centre) are in relative good
agreement, except maybe for the later-type spirals.Comment: 34 pages, 25 figures, accepted for publication in MNRAS. To obtain a
higher resolution version, go to
ftp://ftp.astro.umontreal.ca/outgoing/olivier/bhabar.pdf or to
http://www.astro.umontreal.ca/fantomm/bhabar
Application des connaissances scientifiques en prévention du suicide : Vérification d’une stratégie fondée sur la communauté de pratique
Cet article a pour objectif de décrire une expérience pilote fondée sur les principes d’action des communautés de pratique (CoP), afin de rapprocher chercheurs et milieux de pratique en prévention du suicide et favoriser une meilleure utilisation des connaissances scientifiques. Des professionnels (n = 15) de différents organismes concernés par la prévention du suicide au Québec et disséminés sur tout le territoire (Centres de prévention du suicide, centres jeunesse, direction de santé publique, milieux hospitaliers), ainsi que des chercheurs (n = 4) et un animateur de la communauté ont participé à cette expérience innovante. La CoP a permis d’obtenir des effets sur la réceptivité envers les connaissances, l’accès aux ressources et aux connaissances et le développement de collaboration entre les membres. Des conditions préalables semblent cependant nécessaires à des collaborations accrues entre recherche et pratique, notamment un rapprochement sur le plan des valeurs et une relation fondée sur la confiance et le respect de l’autre et la capacité d’investir du temps dans le développement de relations de travail.The objective of this article is to describe a pilot experiment based on community of practice (CoP) action principles and aimed at bridging the gap between suicide prevention researchers and practitioners and encouraging better utilization of research knowledge. Participants in this innovative experiment included professionals (n = 15) from a variety of Quebec organizations concerned with suicide prevention located throughout the province (suicide prevention centers, youth centers, public health department, hospital settings), researchers (n = 4) and one community animator. The CoP made it possible to obtain effects on receptivity to knowledge, access to resources and knowledge, and the development of collaboration between members. However, it would appear that certain preconditions are necessary for increased collaboration between researchers and practitioners, notably the development of greater common ground in terms of values and a relationship based on trust and mutual respect and the ability to invest time in the development of work relations
On the relevance of the Tremaine-Weinberg method applied to H-alpha velocity field.Pattern speeds determination in M100 (NGC 4321)
The relevance of the Tremaine-Weinberg (TW) method is tested to measure the
bar, spiral and inner structure pattern speeds using a gaseous velocity field.
The TW method is applied to various simulated barred galaxies in order to
demonstrate its validity in seven different configurations, including star
formation or/and dark matter halo. The reliability of the different physical
processes involved and of the various observational parameters are also tested.
The simulations show that the TW method could be applied to the gaseous
velocity fields to get a good estimate of the bar pattern speed, under the
condition that regions of shocks are avoided and measurements are confined to
regions where the gaseous bar is well formed. We successfully apply the TW
method to the \ha velocity field of the Virgo Cluster Galaxy M100 (NGC 4321)
and derive pattern speeds of 55+/-5 km/s/kpc for the nuclear structure, 30+/-2
km/s/kpc for the bar and 20+/-1 km/s/kpc for the spiral pattern, in full
agreement with published determinations using the same method or alternative
ones.Comment: 29 pages, 8 figures, accepted for publication in ApJ. To obtain a
higher resolution version, visit to
http://www.astro.umontreal.ca/fantomm/bhabar
The Evolving Role of Faculty: Traditional Scholarship, Instructional Scholarship and Service Scholarship
Faculty workload decisions made by a departmental unit often create a conflict for faculty because promotion/tenure decisions usually focus primarily on individual scholarly achievements. This paper describes an approach to faculty evaluation that considers both departmental and individual needs by expanding the view of scholarship to include Research, Instruction, and Service
1-Methyl-1-azonia-3,5-diaza-7-phosphaÂtricycloÂ[3.3.1.1]decane 7-oxide triiodide
The title compound, C7H15N3OP+·I3
−, is a derivative of the well known water-soluble aminoÂphosphine 1,3,5-triaza-7-phosphaadamantane (PTA). The crystal structure is composed of a cage-like 1-methyl-1-azonia-3,5-diaza-7-phosphaÂtricycloÂ[3.3.1.1]decane 7-oxide cation and a triiodide anion. The N-methylÂation of the PTA cage results in a slight elongation of the corresponding C—N bonds, while the oxidation of the P atom leads to a slight shortening of the C—P bonds in comparison with those of PTA. In general, most of the bonding parameters are comparable with those reported for related compounds bearing the PTA core. Two interÂmolecular C—H⋯O hydrogen bonds between methylÂene groups and the P=O group are responsible for the linkage of neighbouring cations into linear one-dimensional hydrogen-bonded chains
Automatic Detection of Expanding HI Shells Using Artificial Neural Networks
The identification of expanding HI shells is difficult because of their
variable morphological characteristics. The detection of HI bubbles on a global
scale therefore never has been attempted. In this paper, an automatic detector
for expanding HI shells is presented. The detection is based on the more stable
dynamical characteristics of expanding shells and is performed in two stages.
The first one is the recognition of the dynamical signature of an expanding
bubble in the velocity spectra, based on the classification of an artificial
neural network. The pixels associated with these recognized spectra are
identified on each velocity channel. The second stage consists in looking for
concentrations of those pixels that were firstly pointed out, and to decide if
they are potential detections by morphological and 21-cm emission variation
considerations. Two test bubbles are correctly detected and a potentially new
case of shell that is visually very convincing is discovered. About 0.6% of the
surveyed pixels are identified as part of a bubble. These may be false
detections, but still constitute regions of space with high probability of
finding an expanding shell. The subsequent search field is thus significantly
reduced. We intend to conduct in the near future a large scale HI shells
detection over the Perseus Arm using our detector.Comment: 39 pages, 11 figures, accepted by PAS
H-alpha Kinematics of the SINGS Nearby Galaxies Survey. I
This is the first part of an Halpha kinematics follow-up survey of the SINGS
sample. The data for 28 galaxies are presented. The observations were done on
three different telescopes with FaNTOmM, an integral field photon counting
spectrometer, installed in the respective focal reducer of each telescope. The
data reduction was done through a newly built pipeline with the aim of
producing the most homogenous data set possible. Adaptive spatial binning was
applied to the data cubes in order to get a constant signal-to-noise ratio
across the field of view. Radial velocity and monochromatic maps were generated
using a new algorithm and the kinematical parameters were derived using
tilted-ring models.Comment: 47 pages, 37 figures, accepted for publication in MNRAS. All
high-res. figures are available at
http://www.astro.umontreal.ca/fantomm/sings . An high-res. version of the
article is available at http://www.astro.umontreal.ca/~odaigle/SINGS.pd
1-Methyl-1-azonia-3,5-diaza-7-phosphatricycloÂ[3.3.1.13,7]decane tetraÂfluoroÂborate
The title compound, C7H15N3P+·BF4
− or [PTA-Me][BF4], is the N-methylÂated derivative of the well known water-soluble aminoÂphosphine 1,3,5-triaza-7-phosphaadamantane (PTA). The asymmetric unit consists of a cage-like cation [PTA-Me]+ and a disordered tetraÂfluoroÂborate anion; two F atoms are disordered equally over two sites. A network of weak interÂmolecular C—H⋯F hydrogen bonds results in a three-dimensional supraÂmolecular assembly
Experimental evidence of a natural parity state in Mg and its impact to the production of neutrons for the s process
We have studied natural parity states in Mg via the
Ne(Li,d)Mg reaction. Our method significantly improves the
energy resolution of previous experiments and, as a result, we report the
observation of a natural parity state in Mg. Possible spin-parity
assignments are suggested on the basis of published -ray decay
experiments. The stellar rate of the Ne(,)Mg
reaction is reduced and may give rise to an increase in the production of
s-process neutrons via the Ne(,n)Mg reaction.Comment: Published in PR
Improved 3D Fabry-Perot Data Reduction Techniques
Improved data reduction techniques for 3D data cubes obtained from
Fabry-Perot integral field spectroscopy are presented. They provide accurate
sky emission subtraction and adaptive spatial binning and smoothing. They help
avoiding the effect analogous to the beam smearing, seen in HI radio data, when
strong smoothing is applied to 3D data in order to get the most extended signal
coverage. The data reduction techniques presented in this paper allow one to
get the best of both worlds: high spatial resolution in high signal-to-noise
regions and large spatial coverage in low signal-to-noise regions.Comment: 10 pages, 9 figures, accepted for publication in MNRA
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