نتایج جستجو برای: interstellar magnetic field

تعداد نتایج: 1054697  

Journal: :iranian journal of toxicology 0
حسین سرمدیان hossein sarmadian department of infectious diseases, arak university of medical sciences, arak, iran. رضا قاسمی خواه reza ghasemikhah department of parasitology and mycology, arak university of medical sciences, arak, iran. فاطمه میرمرادی fatemeh mirmoradi general physician, arak university of medical sciences, arak, iran.

background: hydatidosis it is a zoonotic disease which is caused by the larval stages of different species of the tapeworms (cestoda) of genus echinococcus. currently, the surgery is most definitive method of treatment for hydatid cyst, but always there is the risk of leakage or rupture during the surgery, therefore it is considered unreliable method. methods: protoscoleces of hydatid cysts wer...

2008
J. J. Bock D. P. Marrone

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon-borne instrument was launched by CNES from the Swedish Esrange base near Kiruna. In addition to the 143 GHz and 217 GHz frequency bands dedicated to CMB studies, Archeops had one 545 GHz and six 353 GHz bolometers mounted...

1998
M. Colpi R. Turolla S. Zane

Old neutron stars (ONSs) which have radiated away their internal and rotational energy may still shine if accreting the interstellar medium. Rather stringent limits from the analysis of ROSAT surveys indicate that most optimistic predictions on ONSs observability are in excess of a factor as large as ∼ 100. Here we explore two possible evolutionary scenarios that may account for the paucity of ...

Journal: :Astronomy and Astrophysics 2021

Dust polarization is a powerful tool for studying the magnetic field properties in interstellar medium (ISM). However, it does not provide direct measurement of its strength. Different methods havebeen developed which employ both and spectroscopic data order to infer The most widely applied have been by Davis (1951), Chandrasekhar & Fermi (1953) (DCF), Hildebrand et al. (2009) Houde al.(2009) (...

2007
P. C. Frisch

The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun appears to be located in...

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