Isotopologue ratios are anticipated to be one of the most promising signs of life that can be observed remotely. On Earth, carbon isotopes have been used for decades as evidence […]
Spectroscopy
Viscous Heating As The Dominant Heat Source Inside The Water Snowline Of V883 Ori
FU Orionis-type objects(FUors) are embedded protostars that undergo episodes of high accretion, potentially indicating a widespread but poorly understood phase in the formation of low-mass stars.
Spatial Variations of Jovian Tropospheric Ammonia via Ground-Based Imaging
Optical bandpass-filter observations can be simply processed to determine similar horizontal ammonia distributions above the Jovian cloud tops as mid-infrared and microwave observations.
Synthesis Of Urea On The Surface Of Interstellar Water Ice Clusters. A Quantum Chemical Study
Urea is a prebiotic molecule that has been detected in few sources of the interstellar medium (ISM) and in Murchison meteorite. Being stable against ultraviolet radiation and high-energy electron bombardment, […]
Exoplanet Practice: Webb Space Telescope Studies Uranus
Editor’s note: As we look outward at other worlds in other star systems we some major differences – and similarities with regard ot the variety of worlds and how they […]
Charting Circumstellar Chemistry Of Carbon-rich AGB Stars: I. ALMA 3 mm Spectral Surveys
AGB stars are major contributors to the chemical enrichment of the ISM through nucleosynthesis and extensive mass loss.
Optimising Spectroscopic Observations Of Transiting Exoplanets
When observing the atmospheres of transiting exoplanets using high-resolution spectroscopy, one aims to detect well-resolved spectral features with high signal-to-noise ratios (SNR) as is possible today with modern spectrographs.
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems V: Do Self-Consistent Atmospheric Models Represent JWST Spectra? A Showcase With VHS 1256 b
The unprecedented medium-resolution (R=1500-3500) near- and mid-infrared (1-18um) spectrum provided by JWST for the young (120-160Myr) low-mass (12-20MJup) L-T transition (L7) companion VHS1256b has opened new avenues for the in-depth […]
Can Signs Of Life Be Detected On Enceladus?
As astrophysics technology and research continue to advance, one question persists: is there life elsewhere in the universe? The Milky Way galaxy alone has hundreds of billions of celestial bodies, […]
The Carbon-to-Oxygen Ratio in Cool Brown Dwarfs and Giant Exoplanets. I. The Benchmark Late-T dwarfs GJ 570D, HD 3651B and Ross 458C
Measurements of the C/O ratio in brown dwarfs are lacking, in part due to past models adopting solar C/O only. We have expanded the ATMO 2020 atmosphere model grid to […]
