Results 261 to 270 of about 66,681 (291)

Stellar Winds, Magnetic Fields and Disks

2013
All main sequence stars lose mass via stellar winds. The winds of cool stars like the sun are driven by gas pressure gradient. However, the winds of hot massive stars which tend to be luminous are driven by emitted by the star radiation pressure. Mass loss from such winds are significantly higher.
openaire   +1 more source

Jets from MRC 0600-399 bent by magnetic fields in the cluster Abell 3376

Nature, 2021
James O Chibueze, Haruka Sakemi, Takumi Ohmura   +2 more
exaly  

Real-space visualization of intrinsic magnetic fields of an antiferromagnet

Nature, 2022
Takehito Seki, Scott D Findlay, Yuichi Ikuhara   +2 more
exaly  

Stellar magnetic fields

2015
Stefano Bagnulo, John D. Landstreet
openaire   +1 more source

Magnetic fields in stellar radiative interiors

Understanding dynamical processes taking place below the surface of stars is key for a better estimate of stellar ages. The recent measurement of low-and intermediate-mass stars’ slow core rotation during the evolved stages of their evolution shows the need for strong angular momentum transport processes from the core to the envelope. Internal magnetic
openaire   +1 more source

Molecular imaging in oncology: Current impact and future directions

Ca-A Cancer Journal for Clinicians, 2022
Steven P Rowe, Martin G Pomper
exaly  

Multiparametric prostate magnetic resonance imaging in the evaluation of prostate cancer

Ca-A Cancer Journal for Clinicians, 2016
Baris Turkbey, Sandeep Sankineni, Bradford J Wood   +2 more
exaly  

Magnetic Fields of Nondegenerate Stars

Annual Review of Astronomy and Astrophysics, 2009
Jean-François Donati
exaly  

Review of Preoperative Magnetic Resonance Imaging (MRI) in Breast Cancer: Should MRI Be Performed on All Women with Newly Diagnosed, Early Stage Breast Cancer?

Ca-A Cancer Journal for Clinicians, 2009
Nehmat Houssami
exaly  

Stellar magnetic fields

1989
openaire   +1 more source