Results 151 to 160 of about 176,075 (225)
Bar-driven Transport of Molecular Gas in Spiral Galaxies: Observational Evidence [PDF]
The NRO-OVRO CO imaging survey showed that molecular gas was more concentrated to the central kiloparsec in barred spiral galaxies than in their unbarred counterparts. The result provided not only evidence for bar-driven gas transport but also estimates on the mean rate of gas transfer and lower limits to the lifetime of bars.
arxiv
Simulations of cosmic ray propagation. [PDF]
Hanasz M, Strong AW, Girichidis P.
europepmc +1 more source
ALMA-LEGUS. II. The Influence of Subgalactic Environments on Molecular Cloud Properties
We compare the molecular cloud properties in subgalactic regions of two galaxies, barred spiral NGC 1313, which is forming many massive clusters, and flocculent spiral NGC 7793, which is forming significantly fewer massive clusters despite having a ...
Molly K. Finn+26 more
doaj +1 more source
Circumnuclear regions in barred spiral galaxies — I. Near-infrared imaging [PDF]
D. Pérez-Ramírez+5 more
openalex +1 more source
Optical emission line velocities in NGC 1365 are presented along 35 slit positions, of which 18 have not been published earlier. Diagrams of emission line velocities as function of distance along the slits are presented, and separate velocity fields are ...
P. Lindblad+5 more
semanticscholar +1 more source
Abundance gradients in a sample of barred spiral galaxies [PDF]
O. L. Dors, M. V. F. Copetti
openalex +1 more source
Mapping Obscured Star Formation in the Host Galaxy of FRB 20201124A
We present high-resolution 1.5–6 GHz Karl G. Jansky Very Large Array and Hubble Space Telescope (HST) optical and infrared observations of the extremely active repeating fast radio burst (FRB) FRB 20201124A and its barred spiral host galaxy. We constrain
Yuxin Dong+25 more
doaj +1 more source
The Potential-Density Phase-Shift Method for Determining the Corotation Radii in Spiral and Barred Galaxies [PDF]
Xiaolei Zhang, R. Buta
openalex +1 more source
Stellar Bars Form Dark Matter Counterparts in TNG50
Dark matter (DM) bars that shadow stellar bars have been previously shown to form in idealized simulations of isolated disk galaxies, but have yet to be studied in a fully cosmological context.
Neil Ash+3 more
doaj +1 more source
We use 0.1″ observations from the Atacama Large Millimeter Array (ALMA), Hubble Space Telescope (HST), and JWST to study young massive clusters (YMCs) in their embedded “infant” phase across the central starburst ring in NGC 3351.
Jiayi Sun+40 more
doaj +1 more source