This article presents results of VLBI observations of regions of H2O maser activity in the Local Group galaxies M33 and IC 10. Since all position measurements were made relative to extragalactic background sources, the proper motions of the two galaxies could be measured. For M33, this provides this galaxy’s three dimensional velocity, showing that this galaxy is moving with a velocity of 190 ±...

حي ت يو جذومنلأا ىلع يطخلا ريغ أ ،ءاملا ةمدص رث جاوملأاو يلاقتنلاا ه ، ةفاضإ ىلإ ضيف ءا ملا . مب ا نمق ه تءافآو ما ظنلا ة ناتم ة ساردلو أ ة شقان تاز يمملاو تابارط ضلاا ر ث (Parameters) ملا ر يغت ة بُ لطتيو ، مُيم صت ةَ فرعم ما ظنلا اذ ه ي ف ر يغتلا ىد م هذ ه مي ق تازيمملا . ةُقيرط تمدخُتسا دقو H ∞ يف دودحلا ةد يدع ميمصتلا . تا نارتقلاا را بتخا م ت ا مآ لا ة يكيمانيدلا ة ننقملا مكحت لل ة بولطملا ...

We discuss the giant-pulse phenomenon exhibited by pulsars and the distances to which giant pulses might be detected from extragalactic pulsars. We describe the conditions under which a single-pulse search is more sensitive than a standard periodicity search. We find that, for certain pulse-amplitude distribution power laws and time series lengths, single-pulse searches can be superior. We pres...

We present observations of the 492 GHz [CI] emission for four individual giant molecular clouds in the Local Group galaxy M33 obtained with the James Clerk Maxwell Telescope. The average [CI] to CO J=1-0 integrated intensity ratio of 0.10± 0.03 is similar to what is observed in Galactic molecular clouds but smaller than what is seen in starburst galaxies. Similarly, the column density ratio N(C...

هدف: هدف پژوهش حاضر، ساخت و اعتبار­سنجی سیاهه آسیب‌شناسی روانشناختی نوجوانان در فضای مجازی بود. روش: روش آمیخته اکتشافی (کیفی-کمی) بدین منظور با استفاده از تحلیل مضمون مقالات مصاحبه‌های انجام‌شده متخصصان فعال مجازی، آسیب­ ها شناسایی شدند بر اساس آن ­ای ساخته شد. جامعه آماری بخش کیفی شامل مقالات، اساتید دانشگاه­ های اراک، اصفهان، امام خمینی قزوین شهر اراک بودند که نمونه هدفمند آنها انتخاب کمی بو...

Abstract M31 and M33 are the closest spiral galaxies largest members (together with Milky Way) of Local group, which makes them interesting targets for indirect dark matter searches. In this paper we present studies expected sensitivity Cherenkov Telescope Array (CTA) to an annihilation signal from weakly interacting massive particles M33. We show that a 100 h long observation campaign will all...

We present an analysis of the first space-based far-IR-submm observations of M 33, which measure the emission from the cool dust and resolve the giant molecular cloud complexes. With roughly half-solar abundances, M33 is a first step towards young low-metallicity galaxies where the submm may be able to provide an alternative to CO mapping to measure their H2 content. In this Letter, we measure ...