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相关论文: Estimating the Density of Intermediate Size KBOs f…

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We investigate the kinematics and dynamics of the molecular and ionized gas in the host galaxies of three Palomar-Green quasars at low redshifts, benefiting from the archival millimeter-wave interferometric and optical integral field unit…

星系天体物理 · 物理学 2024-09-25 Qinyue Fei , Ran Wang , Juan Molina , Luis C. Ho , Jinyi Shangguan , Franz E. Bauer , Ezequiel Treister

Observations indicate that some of the largest Kuiper Belt Objects (KBOs) have retained volatiles in the gas phase, which implies the presence of an atmosphere that can affect their reflectance spectra and thermal balance. Volatile escape…

地球与行星天体物理 · 物理学 2015-08-19 R. E. Johnson , A. Oza , L. A. Young , A. N. Volkov , C. Schmidt

An abundance decrease in carbon- and oxygen-bearing species relative to dust has been frequently found in planet-forming disks, which can be attributed to an overall reduction of gas mass. However, in the case of TW Hya, the only disk with…

太阳与恒星天体物理 · 物理学 2015-08-06 Fujun Du , Edwin A. Bergin , Michiel R. Hogerheijde

The detections of atomic hydrogen, heavy atoms and ions surrounding the extrasolar giant planet (EGP) HD209458b constrain the composition, temperature and density profiles in its upper atmosphere. Thus the observations provide guidance for…

地球与行星天体物理 · 物理学 2015-06-11 T. T. Koskinen , M. J. Harris , R. V. Yelle , P. Lavvas

Quasar feedback models often predict an expanding hot gas bubble which drives a galaxy-scale outflow. In many circumstances this hot gas radiates inefficiently and is therefore difficult to observe directly. We present an indirect method to…

星系天体物理 · 物理学 2016-03-23 Jonathan Stern , Claude-Andre Faucher-Giguere , Nadia L. Zakamska , Joseph F. Hennawi

In the paper the behavior of density (or specific volume), the heat of evaporation and entropy per molecule for normal and heavy water on their coexistence curves is discussed. The special attention is paid on the physical nature of the…

统计力学 · 物理学 2009-10-26 V. L. Kulinskii , N. P. Malomuzh

Quasar winds can shock and sweep up ambient interstellar medium (ISM) gas, contributing to galactic quenching. We combine and extend past models of energy-conserving shock bubbles around quasars, investigate model implications from an…

星系天体物理 · 物理学 2024-02-19 Patrick B. Hall , E. Weiss , W. N. Brandt , C. J. Mulholland

Aims. In this letter, we calculate for the first time the full transonic hydrodynamic escape of an Earth-like atmosphere. We consider the case of an Earth-mass planet with an atmospheric composition identical to that of the current Earth…

地球与行星天体物理 · 物理学 2019-05-01 C. P. Johnstone , M. L. Khodachenko , T. Lüftinger , K. G. Kislyakova , H. Lammer , M. Güdel

A multi-fluid model for an atomic hydrogen-proton mixture in the upper atmosphere of extrosolar planet is presented when the continuity and momentum equations of each component have been already solved with an energy equation. The particle…

地球与行星天体物理 · 物理学 2011-05-13 J. H. Guo

Is the hydrodynamics of an interacting many-body system fundamentally limited by basic principles of quantum mechanics? Starting with the conjecture that viscosity is at least as large as entropy density (as measured in fundamental units),…

高能物理 - 理论 · 物理学 2017-10-27 Andrew Lucas

We estimate bulk and shear viscosity at finite temperature and baryon densities of hadronic matter within hadron resonance gas model. For bulk viscosity we use low energy theorems of QCD for the energy momentum tensor correlators. For shear…

高能物理 - 唯象学 · 物理学 2015-05-20 Guru Prakash Kadam , Hiranmaya Mishra

Kuiper Belt objects with absolute magnitude less than 3 (radius $\gtrsim$500 km), the dwarf planets, have a range of different ice/rock ratios, and are more rock-rich than their smaller counterparts. Many of these objects have moons, which…

地球与行星天体物理 · 物理学 2016-05-06 Amy C. Barr , Megan E. Schwamb

Transits in the H I 1216 A (Lyman alpha), O I 1334 A, C II 1335 A, and Si III 1206.5 A lines constrain the properties of the upper atmosphere of HD209458b. In addition to probing the temperature and density profiles in the thermosphere,…

地球与行星天体物理 · 物理学 2015-06-11 T. T. Koskinen , R. V. Yelle , M. J. Harris , P. Lavvas

The dynamic behavior of a hard-sphere colloidal suspension was studied by X-ray Photon Correlation Spectroscopy and Small Angle X-ray Scattering over a wide range of particle volume fractions. The short-time mobility of the particles was…

The bolometric radiation from a central body is potentially a powerful driver of atmospheric escape from planets or satellites. When heated above their equilibrium temperatures those satellites, due to their low surface gravity, are be…

地球与行星天体物理 · 物理学 2025-03-25 Matthäus Schulik , James E. Owen , Richard A. Booth , Shun Fai Ling , Shun Ping Wong

Hydrodynamic escape can strip the envelopes of close-in exoplanets, but most observations of atmospheric mass loss to date have been confined to planets orbiting K and M dwarfs. A growing body of detections of atmospheric escape from…

We demonstrate a direct connection between the density profile of a system of ultra-cold trapped bosonic particles in the rapid-rotation limit and its condensate fraction. This connection can be used to probe the crossover from condensed…

软凝聚态物质 · 物理学 2009-11-07 Jairo Sinova , C. B. Hanna , A. H. MacDonald

In the present series of papers we propose a consistent description of the mass loss process. To study the effects of intrinsic magnetic field of a close-orbit giant exoplanet (so-called Hot Jupiter) on the atmospheric material escape and…

地球与行星天体物理 · 物理学 2015-06-12 I. F. Shaikhislamov , M. L. Khodachenko , Yu. L. Sasunov , H. Lammer , K. G. Kislyakova , N. V. Erkaev

We study the transport coefficients of Quark-Gluon-Plasma in finite temperature and finite baryon density. We use AdS/QCD of charged AdS black hole background with bulk-filling branes identifying the U(1) charge as the baryon number. We…

高能物理 - 理论 · 物理学 2008-12-25 Xian-Hui Ge , Yoshinori Matsuo , Fu-Wen Shu , Sang-Jin Sin , Takuya Tsukioka

The viscosity of water induces a vorticity near the free surface boundary. The resulting rotational component of the fluid velocity vector greatly complicates the water wave system. Several approaches to close this system have been…

流体动力学 · 物理学 2020-06-16 D. Eeltink , A. Armaroli , M. Brunetti , J. Kasparian
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