Secular evolution and the formation of pseudobulges in disk galaxies
▪ Abstract The Universe is in transition. At early times, galactic evolution was dominated by
hierarchical clustering and merging, processes that are violent and rapid. In the far future …
hierarchical clustering and merging, processes that are violent and rapid. In the far future …
Physical properties and environments of nearby galaxies
MR Blanton, J Moustakas - Annual Review of Astronomy and …, 2009 - annualreviews.org
We review the physical properties of nearby, relatively luminous galaxies, using results from
newly available massive data sets together with more detailed observations. First, we …
newly available massive data sets together with more detailed observations. First, we …
Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies
M Querejeta, E Schinnerer, S Meidt, J Sun… - Astronomy & …, 2021 - aanda.org
We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct
morphological masks of sub-galactic environments based on Spitzer 3.6 μm images. At the …
morphological masks of sub-galactic environments based on Spitzer 3.6 μm images. At the …
The universal rotation curve of spiral galaxies—I. The dark matter connection
M Persic, P Salucci, F Stel - Monthly Notices of the Royal …, 1996 - academic.oup.com
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs) and
relative surface photometry to investigate the main mass structure properties of spirals, over …
relative surface photometry to investigate the main mass structure properties of spirals, over …
[HTML][HTML] H II regions and the abundance properties of spiral galaxies
We investigate the relationships between the characteristic oxygen abundance, the radial
abundance gradient, and the macroscopic properties of spiral galaxies by examining the …
abundance gradient, and the macroscopic properties of spiral galaxies by examining the …
A classical morphological analysis of galaxies in the Spitzer survey of stellar structure in galaxies (S4G)
RJ Buta, K Sheth, E Athanassoula… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies (S 4 G) is the largest
available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all …
available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all …
The Spitzer Survey of Stellar Structure in Galaxies ()
ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies () is an Exploration Science
Legacy Program approved for the Spitzer post–cryogenic mission. It is a volume-, magnitude …
Legacy Program approved for the Spitzer post–cryogenic mission. It is a volume-, magnitude …
Dynamics of barred galaxies
JA Sellwood, A Wilkinson - Reports on Progress in Physics, 1993 - iopscience.iop.org
Some 30% of disc galaxies have a pronounced central bar features in the disc plane and
many more have weaker features of a similar kind. Kinematic data indicate that the bar …
many more have weaker features of a similar kind. Kinematic data indicate that the bar …
[KİTAP][B] Astrophysical Formulae: Volume I & Volume II: Radiation, Gas Processes and High Energy Astrophysics/Space, Time, Matter and Cosmology
K Lang - 2006 - books.google.com
Kenneth Lang's classic work Astrophysical Formulae.(Vol. I and II) is now available as soft
cover edition in a set. This volume is a reference source of fundamental formulae in physics …
cover edition in a set. This volume is a reference source of fundamental formulae in physics …
What determines the strength and the slowdown rate of bars?
E Athanassoula - Monthly Notices of the Royal Astronomical …, 2003 - academic.oup.com
Isolated barred galaxies evolve by redistributing their angular momentum, which, emitted by
material in the inner disc at resonance with the bar, can be absorbed by resonant material in …
material in the inner disc at resonance with the bar, can be absorbed by resonant material in …