Results 91 to 100 of about 211,954 (220)
COSMOS-Web: The Role of Galaxy Interactions and Disk Instabilities in Producing Starbursts at z < 4
We study of the role of galaxy–galaxy interactions and disk instabilities in producing starburst activity in galaxies out to z = 4. For this, we use a sample of 387 galaxies with robust total star formation rate measurements from Herschel, gas masses ...
Andreas L. Faisst +53 more
doaj +1 more source
Thirty-two bulges of nearby spirals have been observed, to detect misalignment between disk and bulge apparent major axes. Such misalignment is unequivocally present in the majority of observed objects. This may be due to the triaxiality of disks, bulges, or both.
F. Bertola, M. Vietri, W. W. Zeilinger
openaire +1 more source
Constraining dark energy using real and mock galaxy surveys [PDF]
In this thesis, we study how dark energy may be constrained by measurements of large-scale clustering in future galaxy surveys, and through the imprint of a time-varying large-scale potential on the CMB (the integrated Sachs-Wolfe effect).
CAI, YANCHUAN
core
Broad line emission from iron K- and L-shell transitions in the active galaxy 1H 0707-495
Since the 1995 discovery of the broad iron K-line emission from the Seyfert galaxy MCG-6-30-15 (ref. 1), broad iron K lines have been found in emission from several other Seyfert galaxies, from accreting stellar-mass black holes and even from accreting ...
T. Boller +70 more
core +1 more source
The nature and origin of disky elliptical galaxies [PDF]
The observational trend that disky elliptical galaxies exhibit younger luminosity- weighted ages than boxy ellipticals is investigated. The presence of a possible young stellar disk embedded in these galaxies is explored by comparing kinematics derived ...
McDermid, Richard Morgan
core
Towards AMR Simulations of Galaxy Formation [PDF]
Numerical simulations present a fundamental building block of our modern theoretical understanding of the Universe. As such the work in this thesis is primarily concerned with understanding fundamental differences that lie between the different ...
MITCHELL, NIGEL,LEWIS +1 more
core
While massive stars are known to shape galactic ecosystems, their formation has long been assumed to require the high-density environments of inner galactic disks. This paradigm is challenged by mounting evidence of young massive stars in extended galaxy
Pinjian Chen +7 more
doaj +1 more source
Space physiology: Challenges and solutions for a journey to Mars
Experimental Physiology, Volume 111, Issue 9, Page 3863-3869, 1 September 2026.
Damian M. Bailey
wiley +1 more source
The relation between bar formation, galaxy luminosity, and environment
We derive the bar fraction in three different environments ranging from the field to Virgo and Coma clusters, covering an unprecedentedly large range of galaxy luminosities (or, equivalently, stellar masses).
SÁNCHEZ JANSSEN R. +4 more
core
Galaxy Zoo:the dependence of morphology and colour on environment [PDF]
We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 100,000 objects from Galaxy Zoo, the largest sample of visually classified morphologies yet compiled.
Murray, P +32 more
core +1 more source

