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1
On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds
On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds
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On the theory of mass-loss in dwarf galaxies – I. Basic equations and the case of wave/thermal driven winds

Diego Antonio Falceta Gonçalves

Monthly Notices of the Royal Astronomical Society Oxford v. 432, n. 1, p. 589\2013597, jun. 2013

Oxford 2013

Item não circula. Consulte sua biblioteca.(Acessar)

2
Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40
Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40
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Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40

Hektor Monteiro Diego Antonio Falceta Gonçalves

The Astrophysical Journal Chicago v. 738, n. 2, p. 1-10, sept. 2011

Chicago 2011

Item não circula. Consulte sua biblioteca.(Acessar)

3
Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40
Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40
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Three-Dimensional photoionization structure ande distances of planetary nebulae. IV. NGC 40

Hektor Monteiro Diego Antonio Falceta Gonçalves

The Astrophysical Journal Chicago v. 738, n. 2, p. 1-10, sept. 2011

Chicago 2011

Item não circula. Consulte sua biblioteca.(Acessar)

4
Fast magnetic field amplification in the early Universe growth of collisionless plasma instabilities in turbulent media
Fast magnetic field amplification in the early Universe growth of collisionless plasma instabilities in turbulent media
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Fast magnetic field amplification in the early Universe growth of collisionless plasma instabilities in turbulent media

Diego Antonio Falceta Gonçalves Grzegorz Kowal

The Astrophysical Journal Philadelphia v. 808, n. 1, p. 1-15, jul. 2015

Philadelphia 2015

Item não circula. Consulte sua biblioteca.(Acessar)

5
Dynamo in the Intra-Cluster Medium simulation of CGL-MHD turbulent dynamo
Dynamo in the Intra-Cluster Medium simulation of CGL-MHD turbulent dynamo
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Dynamo in the Intra-Cluster Medium simulation of CGL-MHD turbulent dynamo

R Santos-Lima Elisabete Maria de Gouveia dal Pino; A Lazarian; G Kowal; Diego Antonio Falceta Gonçalves; IAU Symposium (274. 2010 Giardini Naxos, Italy)

Bonanno, A.; de Gouveia dal Pino, E.; Kosovichev, A. G., eds Paris: International Astronomical Union, 2011 Advances in plasma astrophysics: Proceedings

Paris International Astronomical Union 2011

Item não circula. Consulte sua biblioteca.(Acessar)

6
MHD turbulence in the intracluster medium
MHD turbulence in the intracluster medium
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MHD turbulence in the intracluster medium

Diego Antonio Falceta Gonçalves G Kowal; Elisabete Maria de Gouveia Dal Pino; R Santos-Lima; S Nakwacki; A Lazarian; IAU General Assembly Beijing, China) 2012 (28.

Montmerle, T., ed Cambridge: Cambridge University Press, 2015 IAU Highlights of Astronomy, v. 16

Cambridge Cambridge University Press 2015

Item não circula. Consulte sua biblioteca.(Acessar)

7
Evolution of magnetic field in the IGM kinetic MHD turbulence
Evolution of magnetic field in the IGM kinetic MHD turbulence
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Evolution of magnetic field in the IGM kinetic MHD turbulence

Reinaldo S. de Lima Elisabete Maria de Gouveia Dal Pino; A Lazarian; D. Falceta Gonçalves; IAU Symposium (259. 2008 Puerto Santiago, Tenerife, Spain)

Strassmeier, K. G.; Kosovichev, A. G.; Beckman, J.E., eds Paris : IAU, 2009 Cosmic magnetic fields: from planets, to stars and galaxies

Paris IAU 2009

Item não circula. Consulte sua biblioteca.(Acessar)

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Deste Autor:

  1. Falceta-Gonçalves, D
  2. Lazarian, A
  3. Kowal, G
  4. IAU Symposium
  5. Dal Pino, E

Neste Assunto:

  1. Campo Magnético
  2. Nebulosas
  3. Plasma
  4. Astrofísica Estelar
  5. Galáxias

  • Realização: ABCD-USP USP   Logos de Redes Sociais: Freepik

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