Evidence and tardive dyskinesia

Soares, Karla Vanessa Souza; McGrath, John J.; Adams, Clive E

doi:10.1016/s0140-6736(96)91525-1

Cited by 14 publications

(8 citation statements)

References 3 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…These are generally an useful tool when one wants to analyze an observed binary sample in order to extract information such as galaxy mass and angular momentum and orbital period and eccentricity. Such a statistical method has been used intensively in the past (e.g., Turner 1976;van Moorsel 1982;Schweizer 1987;Oosterloo 1988;Soares 1990Soares , 1996.…”

Section: Spatial and Projected Separations In Close Pairsmentioning

confidence: 99%

The Identification of Physical Close Galaxy Pairs

Soares¹

2007

Astron J

View full text Add to dashboard Cite

A classification scheme for close pairs of galaxies is proposed. The scheme is motivated by the fact that the majority of apparent close pairs are in fact wide pairs in three-dimensional space. This is demonstrated by means of numerical simulations of random samples of binary galaxies and the scrutiny of the resulting projected and spatial separation distributions.Observational strategies for classifying close pairs according to the scheme are suggested. As a result, physical (i.e., bound and spatially) close pairs are identified.

show abstract

Section: Spatial and Projected Separations In Close Pairsmentioning

confidence: 99%

The Identification of Physical Close Galaxy Pairs

Soares¹

2007

Astron J

View full text Add to dashboard Cite

show abstract

“…For example, it was mentioned that 500 reports of controlled trials of a wide variety of drugs used to prevent or reduce the mental disorder of people taking antipsychotic drugs have been published in peerreviewed journals without giving such information upon which practice can be based with any confidence [2,3]. Although the efforts of medical journals have improved the situation since then, inadequacies are still being published.…”

Section: Rolf Zetterstrommentioning

confidence: 99%

“…As was pointed out by Iain Chalmers and D. G. Altman at the UK Cochrane Centre in Oxford in 1999, many articles, which may also have been published in prestigious medical journals, have such deficiencies in their design and conduct that they are unreliable [1]. For example, it was mentioned that 500 reports of controlled trials of a wide variety of drugs used to prevent or reduce the mental disorder of people taking antipsychotic drugs have been published in peerreviewed journals without giving such information upon which practice can be based with any confidence [2,3]. Although the efforts of medical journals have improved the situation since then, inadequacies are still being published.…”

mentioning

confidence: 99%

CONSORT recommendations to avoid inadequacies in reports published in Acta Paediatrica

Zetterström¹

2005

Acta Paediatrica

View full text Add to dashboard Cite

“…There have been some works [Soares, 1996] with a semi-analytical description of the dynamics of two point galaxies san1,san2,bleh1,bitre,ezo but as far as we know, there have been few attempts to consider the mass variation problem in binary galaxies [Jeans, 1924, Jeans, 1928. The analytical treatment of two interacting galaxies as a two-body problem cannot be considered satisfactorily since one needs to consider the dynamics of binary galaxies with mass loss or mass exchange between them.…”

Section: Introductionmentioning

confidence: 99%

Analytical Model for the Dynamical Motion of the Bulges of Two Interacting Galaxies

López¹,

López²,

Kemp³

2018

View full text Add to dashboard Cite

Two mathematical models of three bodies of variable masses are used to obtain a qualitative description of two interacting galaxies with mass exchange and mass loss. The reference system is centred on the largest body (the most massive galaxy), and the other two bodies are allowed to move around this one under the laws of gravity. The third body, which simulated the mass lost by the second galaxy in the form of a tail, increases its mass due to the mass lost by the second body and follows its trajectory. We are interested in knowing the time evolution of the separation of the two bulges of the interacting galaxies, and the parameters for the analytical models are obtained by running simulations with the GADGET-2 N-body code. The resulting behavior of this distance in our mathematical models is qualitatively in good agreement with that obtained by this code.

show abstract

Evidence and tardive dyskinesia

Cited by 14 publications

References 3 publications

The Identification of Physical Close Galaxy Pairs

The Identification of Physical Close Galaxy Pairs

CONSORT recommendations to avoid inadequacies in reports published in Acta Paediatrica

Analytical Model for the Dynamical Motion of the Bulges of Two Interacting Galaxies

Contact Info

Product

Resources

About