Upgraded Giant Metrewave Radio Telescope timing of NGC 1851A: a possible millisecond pulsar - neutron star system [0.03%]
NGC 1851A的高精度脉冲星计时：关于毫秒脉冲星-中子星系统的证据
A Ridolfi,P C C Freire,Y Gupta et al.
A Ridolfi et al.
In this work, we present the results of 1 yr of upgraded Giant Metrewave Radio Telescope timing measurements of PSR J0514-4002A, a 4.99-ms pulsar in a 18.8-d eccentric ([Formula: see text]) orbit with a massive companion located in the glob...
The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization [0.03%]
C波段全天候 surveys(C-BASS)：全场强度和偏振单像素的参数拟合模拟实验
Luke Jew,Angela C Taylor,Michael E Jones et al.
Luke Jew et al.
The cosmic microwave background (CMB) B-mode signal is potentially weaker than the diffuse Galactic foregrounds over most of the sky at any frequency. A common method of separating the CMB from these foregrounds is via pixel-based parametri...
Sculpting the valley in the radius distribution of small exoplanets as a by-product of planet formation: the core-powered mass-loss mechanism [0.03%]
利用行星形成过程塑造小系外行星半径分布中的山谷：核心驱动的质量损失机制
Akash Gupta,Hilke E Schlichting
Akash Gupta
Recent observations revealed a bimodal radius distribution of small, short-period exoplanets with a paucity in their occurrence, a radius 'valley', around 1.5-2.0 R⊕. In this work, we investigate the effect of a planet's own cooling lumino...
Atmospheric mass loss due to giant impacts: the importance of the thermal component for hydrogen-helium envelopes [0.03%]
巨大撞击导致的大气质量损失：氢氦包层热组分的重要性
John B Biersteker,Hilke E Schlichting
John B Biersteker
Systems of close-in super-Earths and mini-Neptunes display striking diversity in planetary bulk density and composition. Giant impacts are expected to play a role in the formation of many of these worlds. Previous works, focused on the mech...
Jean-Christophe Loison,Valentine Wakelam,Pierre Gratier et al.
Jean-Christophe Loison et al.
We have developed the first gas-grain chemical model for oxygen fractionation (also including sulphur fractionation) in dense molecular clouds, demonstrating that gas-phase chemistry generates variable oxygen fractionation levels, with a pa...
Bayesian cosmic density field inference from redshift space dark matter maps [0.03%]
红移空间暗物质地图的贝叶斯宇宙密度场反演方法
E G Patrick Bos,Francisco-Shu Kitaura,Rien van de Weygaert
E G Patrick Bos
We present a self-consistent Bayesian formalism to sample the primordial density fields compatible with a set of dark matter density tracers after a cosmic evolution observed in redshift space. Previous works on density reconstruction did n...
Bayesian cosmic density field inference from redshift space dark matter maps [0.03%]
红移空间暗物质地图的贝叶斯宇宙密度场反演
E G Patrick Bos,Francisco-Shu Kitaura,Rien van de Weygaert
E G Patrick Bos
We present a self-consistent Bayesian formalism to sample the primordial density fields compatible with a set of dark matter density tracers after a cosmic evolution observed in redshift space. Previous works on density reconstruction did n...
Adrienn Luspay-Kuti,Kathleen Mandt,Kandis-Lea Jessup et al.
Adrienn Luspay-Kuti et al.
In light of the recent New Horizons flyby measurements, we present a coupled ion-neutral-photochemistry model developed for simulating the atmosphere of Pluto. Our model results closely match the observed density profiles of CH4, N2 and the...
A Yalinewich,E Steinberg,T Piran et al.
A Yalinewich et al.
When a star gets too close to a supermassive black hole, it is torn apart by the tidal forces. Roughly half of the stellar mass becomes unbound and flies away at tremendous velocities - around 104 km s-1. In this work, we explore the idea t...
Germán Molpeceres,Albert Rimola,Cecilia Ceccarelli et al.
Germán Molpeceres et al.
Water is one of the most abundant molecules in the form of solid ice phase in the different regions of the interstellar medium (ISM). This large abundance cannot be properly explained by using only traditional low temperature gas-phase reac...