111 citations · 345 across the 11 of their papers we have counts for
12 papers
Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion
Haiyang S. Wang, Anders Johansen, Ziyan Xu +7
Volatile depletion in rocky planets relative to their host stars is commonplace in both the Solar System and exoplanetary systems, yet the connections between planet formation and…
Plausible constraints on the range of bulk terrestrial exoplanet compositions in the Solar neighbourhood
Rob J. Spaargaren, Haiyang S. Wang, Stephen J Mojzsis +2
Rocky planet compositions regulate planetary evolution by affecting core sizes, mantle properties, and melting behaviours. Yet, quantitative treatments of this aspect of exoplanet…
Large Interferometer For Exoplanets (LIFE): VIII. Where is the phosphine? Observing exoplanetary PH3 with a space based MIR nulling interferometer
D. Angerhausen, M. Ottiger, F. Dannert +9
Phosphine could be a key molecule in the understanding of exotic chemistry happening in (exo)planetary atmospheres. While it has been detected in the Solar System's giant planets,…
Detailed chemical compositions of planet-hosting stars: II. Exploration of the interiors of terrestrial-type exoplanets
Haiyang S. Wang, Sascha P. Quanz, David Yong +4
A major goal in the discovery and characterisation of exoplanets is to identify terrestrial-type worlds that are similar to (or otherwise distinct from) our Earth. Recent results h…
The Accretion flow in M87 is really MAD
Feng Yuan, Haiyang Wang, Hai Yang
The supermassive black holes in most galaxies in the universe are powered by hot accretion flows. Both theoretical analysis and numerical simulations have indicated that, depending…
A model Earth-sized planet in the habitable zone of Centauri A/B
Haiyang S. Wang, Charles H. Lineweaver, Sascha P. Quanz +5
The bulk chemical composition and interior structure of rocky exoplanets are of fundamental importance to understanding their long-term evolution and potential habitability. Observ…
Reflection spectra of accretion disks illuminated by disk-like coronae
Shafqat Riaz, Askar B. Abdikamalov, Dimitry Ayzenberg +3
Relativistic reflection features in the X-ray spectra of black hole binaries and AGNs are thought to be produced through illumination of a cold accretion disk by a hot corona. In t…
Europium as a lodestar: diagnosis of radiogenic heat production in terrestrial exoplanets
Haiyang S. Wang, Thierry Morel, Sascha P. Quanz +1
Long-lived radioactive nuclides, such as K, Th, U and U, contribute to persistent heat production in the mantle of terrestrial-type planets. As refra…
Reflection features in the X-ray spectrum of Fairall 9 and implications for tests of general relativity
Honghui Liu, Haiyang Wang, Askar B. Abdikamalov +2
X-ray reflection spectroscopy is potentially a powerful tool to probe the spacetime geometry around astrophysical black holes and test general relativity in the strong field regime…
The Volatility Trend of Protosolar and Terrestrial Elemental Abundances
Haiyang S. Wang, Charles H. Lineweaver, Trevor R. Ireland
We present new estimates of protosolar elemental abundances based on an improved combination of solar photospheric abundances and CI chondritic abundances. These new estimates indi…
The Elemental Abundances (with Uncertainties) of the Most Earth-like Planet
Haiyang S. Wang, Charles H. Lineweaver, Trevor R. Ireland
To first order, the Earth as well as other rocky planets in the Solar System and rocky exoplanets orbiting other stars, are refractory pieces of the stellar nebula out of which the…
Chemical Complementarity between the Gas Phase of the Interstellar Medium and the Rocky Material of Our Planetary System
Haiyang Wang, Charles H. Lineweaver
We compare the elemental depletions in the gas phase of the interstellar medium (ISM) with the elemental depletions in the rocky material of our Solar System. Our analysis finds a…