The Envelopes of Spherical Galaxies

نویسندگان

چکیده

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Environmental Dependence of the Nature of Gaseous Envelopes of Galaxies

We present new statistical study on the origin of Lyα absorption systems that are detected in QSO fields. The primary objective is to investigate environmental dependence of the relationship between galaxies and Lyα absorption systems. We find that galaxies exhibit no environmental dependence in giving rise to Lyα absorbers in their halos. Conversely, Lyα absorbers do not exhibit preference as ...

متن کامل

Merger Rate of Equal-Mass Spherical Galaxies

We present cross sections and reaction rates for merging to occur during encounters of equal-mass spherical galaxies. As an application, we determine the rate of galaxy merging in clusters of galaxies. We present results for two types of Plummer models (a full and a truncated one), two King models and the Hernquist model. Cross sections are determined on the basis of a large number (∼ 500) of s...

متن کامل

Green envelopes classification: the comparative analysis of efficient factors on the thermal and energy performance of green envelopes

This paper classifies green envelopes as green roofs and green walls according to effective factors, which were derived from literature to compare the green envelopes’ thermal and energy performance in a more effective way. For this purpose, an extensive literature review was carried out by searching keywords in databases and studying related journal papers and articles. The research meth...

متن کامل

Spherical Accretion in Nearby Weakly Active Galaxies

We consider the sample of weakly active galaxies situated in ’Local Universe’ collected in the paper of Pellegrini (2005) with inferred accretion efficiencies from 10−2 to 10−7. We apply a model of spherically symmetrical Bondi accretion for given parameters (MBH ,T∞,ρ∞,) taken from observation. We calculate spectra emitted by the gas accreting onto its central objects using Monte Carlo method ...

متن کامل

Stellar Populations in the Central Galaxies of Fossil Groups

It is inferred from the symmetrical and luminous X-ray emission of fossil groups that they are mature, relaxed galaxy systems. Cosmological simulations and observations focusing on their dark halo and inter-galactic medium properties confirm their early formation. Recent photometric observations suggest that, unlike the majority of non-fossil brightest group galaxies (BGGs), the central early-t...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Symposium - International Astronomical Union

سال: 1987

ISSN: 0074-1809

DOI: 10.1017/s0074180900185997