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    Probing the local bubble with diffuse interstellar bands

    , Article Proceedings of the International Astronomical Union ; Vol. 9, issue. S297 , February , 2014 , pp. 84-88 ; ISSN: 17439213 Farhang, A ; Khosroshahi, H. G ; Javadi, A ; Van Loon, J ; Sharif University of Technology
    Abstract
    The Sun is located inside an enormous local cavity filled with a million degree, ionized hydrogen gas and surrounded by a wall of dense and cold gas, this cavity is known as the Local Bubble (LB). Since the tempreture of Local Bubble is high, the typical singly-ionized atoms or molecules can not survive at this high tempreture. To overcome this problem we should probe the Local Bubble using species which survive under this condition so we have done a whole sky survey in north hemisphere by observing absorptions in the Diffuse Interstellar Bands (DIBs) for sight-lines with distance >300 pc. We have done 30 nights observation and have observed 473 bright stars. We found that the correlations... 

    Simulation of optical interstellar scintillation

    , Article Astronomy and Astrophysics ; Volume 552, Article No. A93 , 2013 ; 00046361 (ISSN) Habibi, F ; Moniez, M ; Ansari, R ; Rahvar, S ; Sharif University of Technology
    2013
    Abstract
    Aims. Stars twinkle because their light propagates through the atmosphere. The same phenomenon is expected on a longer time scale when the light of remote stars crosses an interstellar turbulent molecular cloud, but it has never been observed at optical wavelengths. The aim of the study described in this paper is to fully simulate the scintillation process, starting from the molecular cloud description as a fractal object, ending with the simulations of fluctuating stellar light curves. Methods. Fast Fourier transforms are first used to simulate fractal clouds. Then, the illumination pattern resulting from the crossing of background star light through these refractive clouds is calculated... 

    Searching for galactic hidden gas through interstellar scintillation: Results from a test with the NTT-SOFI detector

    , Article Astronomy and Astrophysics ; Volume 525, Issue 6 , 2010 ; 00046361 (ISSN) Habibi, F ; Moniez, M ; Ansari, R ; Rahvar, S ; Sharif University of Technology
    2010
    Abstract
    Aims. Stars twinkle because their light propagates through the atmosphere. The same phenomenon is expected at a longer time scale when the light of remote stars crosses an interstellar molecular cloud, but it has never been observed at optical wavelength. In a favorable case, the light of a background star can be subject to stochastic fluctuations on the order of a few percent at a characteristic time scale of a few minutes. Our ultimate aim is to discover or exclude these scintillation effects to estimate the contribution of molecular hydrogen to the Galactic baryonic hidden mass. This feasibility study is a pathfinder toward an observational strategy to search for scintillation, probing...