Bulge formation through disc instability

نویسندگان
چکیده

برای دانلود رایگان 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

Bulge Formation

The currently discussed theories of bulge formation are reviewed, including the pri-mordial scenario, where bulges form rapidly and then accrete disks, the secular scenario, where bulges are formed by dynamical evolution of disks through bars and galaxy interactions , and some combinations of both, where formation of bulges and disks are more continuous and interleaved. The various scenarios ma...

متن کامل

Planetesimal Formation through Gravitational Instability

Introduction. Two prevailing processes of planetesimal formation are proposed. The first is the gravitational instability of a dust layer (e.g., Safronov 1969, Hayashi 1972, Goldreich and Ward 1973). The second is the growth through the mutual sticking of dust particles in a turbulent nebula (Weidenschilling and Cuzzi 1993, Stepinski and Valageas 1997). We consider the first one in this study. ...

متن کامل

Gravitational instability and star formation in disc galaxies

We present a general star formation law in which the star formation rate depends upon the ef®ciency a and the time-scale t of star formation, and the gas component jg of the surface mass density. The current nominal Schmidt exponent nS for our model is 2 < nS < 3. Based on a gravitational instability parameter QA and another dimensionless parameter fP ˆ …P=Gj 2 c† , where P ˆ pressure and jc ˆ ...

متن کامل

The Disc Origin of the Milky Way Bulge

The Galactic bulge, that is the prominent out-of-plane over-density present in the inner few kiloparsecs of the Galaxy, is a complex structure, as the morphology, kinematics, chemistry, and ages of its stars indicate. To understand the nature of its main components—those at [Fe/H] −1 dex—it is necessary to make an inventory of the stellar populations of the Galactic disc(s), and of their border...

متن کامل

Chiari Formation: Atlantoaxial Instability is the Cause

The entity of Chiari formation was&nbsp;described by Hans Chiari in 1891 [1,2].&nbsp;Since then the subject has been evaluated&nbsp;elaborately by a number of authors. However,&nbsp;it may only be correct to state that confusion&nbsp;in the understanding of pathogenesis and the&nbsp;nature of anomaly, significance of associated&nbsp; abnormal soft tissue and bone anomalies&nbsp;and more importa...

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: Astronomy & Astrophysics

سال: 2020

ISSN: 0004-6361,1432-0746

DOI: 10.1051/0004-6361/201936439