Photometric investigations of NGC 2577 and NGC 4310 Lenticular Galaxies
In this study, two lenticular galaxies ( NGC 2577, NGC 4310 ) have been chosen to study their morphological and photometric properties, by using The [1] IRAF ISOPHOTE ELLIPSE task with griz -Filters.
Abdullah K Ahmed, Zahraa Adnan
semanticscholar +1 more source
Globular clusters and planetary nebulae kinematics and X-ray emission in the early-type galaxy NGC 5128 [PDF]
The estimates of the mass of the galaxy NGC 5128 based on the different mass tracers, globular clusters (GCs) and planetary nebulae (PNe), are presented.
Samurović S.
doaj +1 more source
The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the Fundamental Plane of elliptical and lenticular galaxies [PDF]
We investigate the well-known correlations between the dynamical mass-to-light ratio M/L and other global observables of elliptical (E) and lenticul ar (S0) galaxies.
M. Cappellari +14 more
semanticscholar +1 more source
The total mass of the early-type galaxy NGC 4649 (M60) [PDF]
In this paper the problem of the total mass and the total mass-to-light ratio of the early-type galaxy NGC 4649 (M60) is analyzed. Use is made of two independent techniques: the X-ray methodology which is based on the temperature of the X-ray halo of NGC
Samurović S., Ćirković M.M.
doaj +3 more sources
Galaxy formation and evolution are hierarchical. The most massive galaxies are thought to form their central regions early through violent dissipational processes, then grow inside-out by accreting smaller satellites.
Haoran Dou +4 more
doaj +1 more source
Star Formation in the Lopsided Galaxy Arp 291
We have investigated the star formation process taking place in the lopsided galaxy Arp 291, based on narrowband images in the H α , [N ii ] λ 6583, and [O iii ] λ 5007 emission lines, obtained using the modern tunable photometer MaNGaL at the Caucasus ...
Irina S. Proshina, Dmitriy V. Oparin
doaj +1 more source
Spectroscopic bulge-disc decomposition: a new method to study the evolution of lenticular galaxies [PDF]
A new method for spectroscopic bulge–disc decomposition is presented, in which the spatial light profile in a two-dimensional spectrum is decomposed wavelength by wavelength into bulge and disc components, allowing separate one-dimensional spectra for ...
E. Johnston +3 more
semanticscholar +1 more source
Understanding the Fundamental Plane and the Tully Fisher Relation
The relation between early type galaxy size, surface brightness and velocity dispersion, “the fundamental plane,” has long been understood as resulting from equilibrium in their largely pressure supported stellar dynamics.
Jeremy Mould
doaj +1 more source
PGC 44685: A Dwarf Star-forming Lenticular Galaxy with a Wolf–Rayet Population
Lenticular galaxies (S0s) are formed mainly from the gas stripping of spirals in the cluster. But how S0s form and evolve in the field is still in need of being resolved.
Shiying Lu +10 more
doaj +1 more source
Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535
Lenticular galaxies (S0s) in the local Universe are generally absent of recent star formation and lack molecular gas. In this paper, we investigate one massive ( M _* ∼ 5 × 10 ^10 M _⊙ ) star-forming S0, PGC 39535, with the Northern Extended Millimeter ...
Jiantong Cui +5 more
doaj +1 more source

