Results 201 to 210 of about 1,782 (230)

One month convection timescale on the surface of a giant evolved star. [PDF]

Nature
Vlemmings W, Khouri T, Bojnordi Arbab B, De Beck E, Maercker M.   +4 more
europepmc   +1 more source

Smartphone-Based Hand Function Assessment: Systematic Review.

J Med Internet Res
Fu Y, Zhang Y, Ye B, Babineau J, Zhao Y, Gao Z, Mihailidis A.   +6 more
europepmc   +1 more source

AptERA 2 targets ERA from Staphylococcus aureus and limits GTP hydrolysis

Peñaranda K, Pereira N, Savva O, Petrelli D, Spurio R, Corrigan RM, Milon P.   +6 more
europepmc   +1 more source

The multiwavelength behaviour of BL Lacertae explained by a wiggling filamentary jet

Raiteri C.
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

The Rotation Curve of our Galaxy

Applied Mechanics and Materials, 2014
The rotation curve of our Galaxy is derived from a large sample of objects with known radial velocities and distances. We collect data as completely as possible, especially the data with accurately measured trigonometric parallaxes. These observations are used to construct a highly accurate rotation curve of the Galaxy.
Gui Ping Ruan, Wei Bin Shi
openaire   +2 more sources

The Rotation Curve of the Galaxy

1983
The determination of the rotation curve of the Galaxy, θ(R), where θ is the circular velocity at galactocentric distance R, involves the synthesis of a large body of complementary (and sometimes contradictory) data. The synthesis has to be guided to some extent by theoretical considerations such as studying the distribution of mass in the Galaxy, i.e ...
openaire   +2 more sources

The Dynamics of Galaxy Rotational Curves

Space 2006, 2006
During the 1980’s, the first astronomical evidence was obtained that appeared to indicate spiral galaxies, (see Figure 1) do not rotate according to Newton’s’ Second Law of Motion: F=MA. The observations suggest that the outer stars in galaxies seem to rotate too fast for the amount of matter we see in the galaxy.
openaire   +2 more sources

The kinematic effects on the rotation curve of a galaxy

Astrophysics and Space Science, 1988
In this paper, it is pointed out that if the spiral galaxy revolves about some common centre as a whole, the rotation curve will be changed by the kinematic effects. The common centre could be the centre of supercluster or the centre of dark matter and luminous matter.
Chongming Xu, Xuejun Wu
openaire   +2 more sources

Auto‐Switching Self‐Powered System for Efficient Broad‐Band Wind Energy Harvesting Based on Dual‐Rotation Shaft Triboelectric Nanogenerator

Advanced Energy Materials, 2021
Jiyu Wang, Zhong Lin Wang
exaly  

NIR Light‐Driving Barrier‐Free Group Rotation in Nanoparticles with an 88.3% Photothermal Conversion Efficiency for Photothermal Therapy

Advanced Materials, 2020
Xiaojun Peng, Vinod Kumar, Wen Sun
exaly