Results 81 to 90 of about 8,619 (233)
Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
We review internal processes of secular evolution in galaxy disks, concentrating on the buildup of dense central features that look like classical, merger-built bulges but that were made slowly out of disk gas. We call these pseudobulges. As an existence
Arp H +95 more
core +2 more sources
The CO-to-H2 Conversion Factor in the Barred Spiral Galaxy M83
We analyze the CO-to-H _2 conversion factor ( α _CO ) in the nearby barred spiral galaxy M83. We present new H i observations from the VLA and single-dish GBT in the disk of the galaxy, and combine them with maps of CO(1-0) integrated intensity and dust ...
Amanda M Lee +4 more
doaj +1 more source
Chemical enrichment in isolated barred spiral galaxies [PDF]
16 pages, 11 figures, accepted for publication in ...
Hugo Martel +4 more
openaire +2 more sources
N‐terminal betaine conjugation modifies β‐peptide helices, influencing folding and self‐organization. For [1S, 2S]‐ACPC, folding to an H12 helix was unaffected, while [1R, 2R]‐ACHC formed an H14 helix instead of H10. Alternating heterochiral oligomers made of enantiomeric pairs of trans‐ACPC showed enhanced solubility and E‐strand formation.
Nikolett Varró +10 more
wiley +1 more source
Stellar Populations, Bars and Secular Evolution in Late-Type Galaxies [PDF]
We have done a robust statistical analysis of UBV color profiles of 257 Sbc barred and unbarred galaxies. We found that there is an excess of barred galaxies among the objects with null or positive (bluish inward) color gradients, which seems to indicate
Corsini, Enrico Maria +3 more
core +1 more source
AGN spiral galaxies in groups: effects of bars [PDF]
We explore properties of barred active spiral galaxies in groups selected from the SDSS-DR7, with the aim of assessing the effects of bars on AGN and the role of the high density environment.
Alonso, Sol +2 more
core +1 more source
Impacts of Bar-driven Shear and Shocks on Star Formation
Bars drive gas inflow. As the gas flows inward, shocks and shear occur along the bar dust lanes. Such shocks and shear can affect the star formation (SF) and change the gas properties.
Taehyun Kim +14 more
doaj +1 more source
Despite the 30 yr history of ultraluminous X-ray sources (ULXs) studies, issues such as the majority of their physical natures (i.e., neutron stars, stellar-mass black holes, or intermediate black holes) as well as the accretion mechanisms are still ...
Chen-Hsun Ma +3 more
doaj +1 more source
Formation of Nuclear Spirals in Barred Galaxies [PDF]
38 pages, 10 figures, accepted for publication in ...
Ann, H. B., Thakur, Parijat
openaire +2 more sources

