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期刊名:Nature astronomy

缩写:NAT ASTRON

ISSN:2397-3366

e-ISSN:2397-3366

IF/分区:15.2/Q1

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共收录本刊相关文章索引81
Clinical Trial Case Reports Meta-Analysis RCT Review Systematic Review
Classical Article Case Reports Clinical Study Clinical Trial Clinical Trial Protocol Comment Comparative Study Editorial Guideline Letter Meta-Analysis Multicenter Study Observational Study Randomized Controlled Trial Review Systematic Review
Stephanie L Yardley,David H Brooks,Raffaella D&#x;Amicis et al. Stephanie L Yardley et al.
The ambient solar wind that fills the heliosphere originates from multiple sources in the solar corona and is highly structured. It is often described as high-speed, relatively homogeneous, plasma streams from coronal holes and slow-speed, ...
Merav Opher,Abraham Loeb,J E G Peek Merav Opher
Cold, dense clouds in the interstellar medium of our Galaxy are 4-5 orders of magnitude denser than their diffuse counterparts. Our Solar System has most likely encountered at least one of these dense clouds during its lifetime. However, ev...
Taylor J Bell,Nicolas Crouzet,Patricio E Cubillos et al. Taylor J Bell et al.
Hot Jupiters are among the best-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models predict that clouds may condense on the nightside and that mol...
Peter K Blanchard,V Ashley Villar,Ryan Chornock et al. Peter K Blanchard et al.
Identifying the sites of r-process nucleosynthesis, a primary mechanism of heavy element production, is a key goal of astrophysics. The discovery of the brightest gamma-ray burst (GRB) to date, GRB 221009A, presented an opportunity to spect...
Harry A Ballantyne,Erik Asphaug,C Adeene Denton et al. Harry A Ballantyne et al.
Pluto's surface is dominated by the huge, pear-shaped basin Sputnik Planitia. It appears to be of impact origin, but modelling has not yet explained its peculiar geometry. We propose an impact mechanism that reproduces its topographic shape...
Gregory Desvignes,Patrick Weltevrede,Yong Gao et al. Gregory Desvignes et al.
Magnetars-highly magnetized neutron stars-are thought to be the most likely progenitors for fast radio bursts (FRBs). Freely precessing magnetars are further invoked to explain the repeating FRBs. We report here on new high-cadence radio ob...
J R Szalay,F Allegrini,R W Ebert et al. J R Szalay et al.
Jupiter's moon Europa has a predominantly water-ice surface that is modified by exposure to its space environment. Charged particles break molecular bonds in surface ice, thus dissociating the water to ultimately produce H2 and O2, which pr...
Remo Burn,Christoph Mordasini,Lokesh Mishra et al. Remo Burn et al.
The radius valley (or gap) in the observed distribution of exoplanet radii, which separates smaller super-Earths from larger sub-Neptunes, is a key feature that theoretical models must explain. Conventionally, it is interpreted as the resul...
Trevor A Bowen,Stuart D Bale,Benjamin D G Chandran et al. Trevor A Bowen et al.
The dissipation of turbulence in astrophysical systems is fundamental to energy transfer and heating in environments ranging from the solar wind and corona to accretion disks and the intracluster medium. Although turbulent dissipation is re...
Lingzhi 灵芝 Wang王,Maokai Hu,Lifan Wang et al. Lingzhi 灵芝 Wang王 et al.
Dust associated with various stellar sources in galaxies at all cosmic epochs remains a controversial topic, particularly whether supernovae play an important role in dust production. We report evidence of dust formation in the cold, dense ...