ABSTRACT There is evidence that the star formation process linked to intricate net of filaments in molecular clouds, which may be also due gas compression from external triggers. We studied southern region Perseus NGC 1333 cloud, known heavily shaped by similar triggers, shed light on perturbed filament where Class 0 IRAS4 protostars lie. use new IRAM-NOEMA observations SiO and CH3OH, both trac...

The coupled utilization of solar and thermal energy is considered an efficient way to improve the efficiency CO2 reduction. Herein, palygorskite (Pal) clay as a silicon source, while Co2+ introduced prepare two-dimensional Co2SiO4 nanosheets, excess leads growth Co3O4 on surface obtain S-scheme Co2SiO4/Co3O4−x heterojunction, which facilitates charge transfer maintains higher redox potentials. ...

We present the results of a multiline survey at mm-wavelengths of the Cepheus A star forming region. Four main flows have been identified: three pointing in the SW, NE, and SE directions and accelerating high density CS clumps. The fourth outflow, revealed by high-sensitivity HDO observations, is pointing towards South and is associated with conditions particularly favourable to a chemical enri...

the date of receipt and acceptance should be inserted later Abstract. We report high angular resolution (HPBW∼ 0.6 ′′ × 0.5 ′′ at 1.3mm) observations of the Class 0 intermediate-mass (IM) protostar NGC 7129–FIRS 2 using the Plateau de Bure Interferometer. Our observations show the existence of an intense unresolved source in the continuum at 1.3mm and 3mm at the position of the Class 0 object. ...

We obtained high resolution (λ/δλ∼ 10,000–20,000) infrared (IR) spectra of Comet 21P/Giacobini–Zinner (GZ) at five different wavelengths between 1.9 and 5.0 μm during 25–29 October 1998 using CSHELL at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. We also obtained a moderate resolution (λ/δλ∼ 680) spectrum covering the wavelength range from 3.082 to 3.720 μm on 29 October 1998 using...

Understanding the ultrafast dynamics of photoexcited carriers at semiconductor/molecule interface is essential for improving solar energy conversion efficiency. At such interfaces, hydrogen bond (H-bond) network often formed, and quantum proton motion expected. However, how nuclear effects (NQEs) will influence charge transfer still unknown. By combining two kinds emerging molecular methods ab ...