Gas Feedback on Stellar Bar Evolution

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

Dating Secular Evolution: Bar Ages from Stellar Kinematics

The last few years witnessed a change of perspective in the context of galaxy formation and evolution. The major role played by bars in the history of these fundamental building blocks of our universe was finally realized. However, and despite the fact that one of the major concerns of any physical science is to measure timescales for natural phenomena, we have as yet no established way to esti...

متن کامل

Dense Molecular Gas: A Sensitive Probe of Stellar Feedback Models

We show that the mass fraction of giant molecular cloud (GMC) gas (n 100 cm−3) in dense (n 104 cm−3) star-forming clumps, observable in dense molecular tracers (LHCN/LCO(1–0)), is a sensitive probe of the strength and mechanism(s) of stellar feedback, as well as the star formation efficiencies in the most dense gas. Using high-resolution galaxy-scale simulations with pc-scale resolution and exp...

متن کامل

The Role of Stellar Feedback in Galaxy Evolution

THE ROLE OF STELLAR FEEDBACK IN GALAXY EVOLUTION

متن کامل

Gas-driven Evolution of Stellar Orbits in Barred Galaxies

We carry out a detailed orbit analysis of gravitational potentials selected at different times from an evolving self-consistent model galaxy consisting of a two-component disk (stars+gas) and a live halo. The results are compared with a pure stellar model, subject to nearly identical initial conditions, which are chosen as to make the models develop a large scale stellar bar. The bars are also ...

متن کامل

The Stellar , Gas And

We present analysis of the near-infrared spectra of 114 rest-frame UV-selected star-forming galaxies at z ∼ 2. By combining the Hα spectra with photometric measurements from observed 0.3–8 μm, we assess the relationships between kinematics, dynamical masses, inferred gas fractions, and stellar masses and ages. The Hα line widths give a mean velocity dispersion σ = 101 ± 5 km s and a mean dynami...

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: The Astrophysical Journal

سال: 2007

ISSN: 0004-637X,1538-4357

DOI: 10.1086/520531