Keywords: ISM: مولکول ها; Stars: formation; ISM: clouds; ISM: molecules; Submillimeter: ISM;
مقالات ISI ISM: مولکول ها (ترجمه نشده)
مقالات زیر هنوز به فارسی ترجمه نشده اند.
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در صورتی که به ترجمه آماده هر یک از مقالات زیر نیاز داشته باشید، می توانید سفارش دهید تا مترجمان با تجربه این مجموعه در اسرع وقت آن را برای شما ترجمه نمایند.
Keywords: ISM: مولکول ها; ISM: molecules; Collisional rate coefficients; H2CO-molecule;
Keywords: ISM: مولکول ها; Astrochemistry; ISM: molecules; ISM: abundances; ISM: evolution; Method: numerical;
Keywords: ISM: مولکول ها; Astrochemistry; ISM: abundances; ISM: molecules;
Keywords: ISM: مولکول ها; Astrochemistry; Methods: laboratory: solid state; ISM: molecules; Comets: general; Infrared: general;
Keywords: ISM: مولکول ها; ISM: molecules; H2CS; H2CSi; Collisional rate coefficients;
Keywords: ISM: مولکول ها; Astrochemistry; Molecular cloud; ISM: molecules; ISM: abundances
Keywords: ISM: مولکول ها; Astrochemistry; Spectra; ISM: molecules; ISM: abundances
Keywords: ISM: مولکول ها; ISM: molecules; Cyclopropenone; Einstein A-coefficients; Radiative transfer;
Keywords: ISM: مولکول ها; Astrochemistry; Molecular processes; Methods: laboratory; Techniques: spectroscopic; ISM: molecules;
Keywords: ISM: مولکول ها; ISM: Molecules; TiH2; Einstein A-coefficients; Radiative transfer
Strengths of rotational lines from H2CC molecule: Addressing tentative detection
Keywords: ISM: مولکول ها; ISM: Molecules; H2CC Molecule; Einstein A-coefficients; Molecular data;
Molecular Lines of CO Isotopes of the High Galactic Latitude Cloud HSVMT27
Keywords: ISM: مولکول ها; ISM: molecules; stars: formation; ISM: kinematics and dynamics;
Ro-vibrational analysis of SiO in UV-irradiated environments
Keywords: ISM: مولکول ها; ISM: molecules; Photodissociation region (PDR); Molecular data; Stars: AGB and post-AGB;
Photodissociation threshold and emission with 220Â nm of icy ethene
Keywords: ISM: مولکول ها; Astrochemistry; Molecular processes; ISM: molecules; UV: ISM; Methods: laboratory;
Frequency Calibration of Spectral Observation System of the TM65m Radio Telescope
Keywords: ISM: مولکول ها; techniques: photometry; spectral line: identification; radio lines: ISM; ISM: molecules;
Optical spectrum of Si3C, and a re-analysis of the Câ¼1B1âXâ¼1A1 transition
Keywords: ISM: مولکول ها; ISM: molecules; Molecular data; Optical spectrum;
Suggestion for search of H2CSi molecule in the interstellar medium
Keywords: ISM: مولکول ها; ISM: molecules; H2CSi molecule; Molecular data
Collisional rates for rotational transitions in H2CO and their application
Keywords: ISM: مولکول ها; ISM: molecules; H2CO molecule; Collisional rates
Importance of collisional rates for anomalous absorption in H2CC molecule
Keywords: ISM: مولکول ها; ISM: molecules; Radiative transfer
Chemical evolution during the process of proto-star formation by considering a two dimensional hydrodynamic model
Keywords: ISM: مولکول ها; Astrochemistry; Star formation; ISM: molecules; ISM: abundances; ISM: evolution; Methods: numerical
Importance of collisional rates for anomalous absorption in H2CO molecule
Keywords: ISM: مولکول ها; ISM: Molecules; H2CO; Transfer of radiation;
Suggestion for the search of H2CC in cool cosmic objects
Keywords: ISM: مولکول ها; ISM: molecules
On the 3D structure of the nebula around η-Carinae
Keywords: ISM: مولکول ها; ISM: molecules; Stars: individual: η-Carinae; Stars: mass loss; Stars: winds; Outflows;
Spectral survey of molecular cores NGC 6334I and NGC 6334I(N) in the range 80.5–242.0 GHz
Keywords: ISM: مولکول ها; ISM: individual (NGC 6334I, NGC 6334I(N)); ISM: molecules; Line: identification; Radiolines: ISM
Carbon monoxide observations of small dark globules: II. Stability analysis
Keywords: ISM: مولکول ها; 98.38.Dq; 33.20.ât; 47.50.Gj; 94.05.Lk; ISM: clouds; ISM: molecules; Instabilities; Turbulence;
Large-scale molecular shocks in galaxies
Keywords: ISM: مولکول ها; Galaxies: individual: NGC 253; Galaxies: individual: IC 342; Galaxies: individual: M 82; Galaxies: starburst; Galaxies: nuclei; ISM: molecules; Molecular processes; Radio lines: galaxies
Molecular gas properties in interacting and merging galaxies
Keywords: ISM: مولکول ها; Galaxies: starburst; Galaxies: active; Radio lines: ISM; ISM: molecules
Amino acids formed from the UV/EUV irradiation of inorganic ices of astrophysical interest
Keywords: ISM: مولکول ها; Molecular processes; Methods: data analysis; ISM: molecules;
Astronomical searches for nitrogen heterocycles
Keywords: ISM: مولکول ها; Astrobiology; Astrochemistry; ISM: chemistry; ISM: molecules; Stars: AGB and post-AGB;