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Time evolution of accreting magnetofluid around a compact object-Newtonian analysis

- F. Habibi, M. Shaghaghian, R. Pazhouhesh
- Physics
- 12 August 2015

Time evolution of a thick disc with finite conductivity around a nonrotating compact object is presented. Along with the Maxwell equations and the Ohm's law, the Newtonian limit of the relativistic… Expand

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Observations, light curves analysis and pulsation behavior of the Algol-type eclipsing binary system XX Cep

- B. Hosseinzadeh, R. Pazhouhesh, K. Yakut
- Physics
- 1 February 2014

Abstract We present the long term photometric variations of the classical Algol type binary XX Cep with a δ Scuti type pulsating component. Modeling of the system shows that the secondary component… Expand

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Self‐similar evolutionary solutions for an accreting magneto‐fluid around a compact object with finite electrical conductivity

- F. Habibi, R. Pazhouhesh, M. Shaghaghian
- Physics
- 1 February 2015

In this paper, we investigate the time evolution of an accreting magneto-fluid with finite conductivity. For the case of a thin disk, the fluid equations along with Maxwell's equations are derived in… Expand

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New Elements of the contact binary V839 Ophiuchi

- R. Pazhouhesh, M. Edalati
- Physics
- 1 February 2002

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Radial Velocity and Light Curves Analysis of the Contact Binary V1073 Cygni

- M. Jafari, B. Khalesseh, R. Pazhouhesh
- Physics
- 15 November 2006

In this study complete BV light curves of the W Ursae Majoris binary V1073 Cygni obtained in 2005 are presented. We have used the spectroscopic data of V1073 Cyg obtained by Ahn et al. (1992) for… Expand

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Radial Velocity and Light Curves Analysis of the Eclipsing Binary V1425 Cygni

- R. Pazhouhesh, M. Jafari, B. Khalesseh
- Physics
- 1 August 2007

The Effect of Dark Matter on Stars at the Galactic Center: The Paradox of Youth Problem

- E. Hassani, R. Pazhouhesh, H. Ebadi
- Physics
- 27 March 2020

Stars that evolve near the Galactic massive black hole show strange behaviors. The spectroscopic features of these stars show that they must be old. But their luminosities are much higher than the… Expand

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Cosmological constrains on new generalized Chaplygin gas model

- Fataneh Salahedin, R. Pazhouhesh, M. Malekjani
- Physics
- 21 May 2020

We use different combinations of data samples to investigate the new generalized Chaplygin gas (NGCG) model in the context of dark energy (DE) cosmology. Using the available cosmological data, we put… Expand

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Period change of binary pulsars due to the accretion of dark matter particles

- E. Hassani, H. Ebadi, R. Pazhouhesh
- Physics
- 3 October 2020

As binary systems move inside galaxies, they interact with the dark matter halo. This interaction leads to the accretion of dark matter particles inside binary components. The accretion of dark… Expand

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