Dense molecular gas around massive young stars |
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HERSCHELHIFI OBSERVATIONS OF O2TOWARD ORION: SPECIAL CONDITIONS FOR SHOCK ENHANCED EMISSION |
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HERSCHELMEASUREMENTS OF MOLECULAR OXYGEN IN ORION |
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HERSCHELOBSERVATIONS OF INTERSTELLAR CHLORONIUM |
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Interstellar absorption features toward the compact infrared source W33A |
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Interstellar absorption lines in the infrared spectrum of NGC 2024 IRS 2 |
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Interstellar absorption lines toward NGC 2264 and AFGL 2591: abundances of H3, H+3, and CO |
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Interstellar C_3_ toward HD 210121 |
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Interstellar CH absorption in the diffuse interstellar medium along the sight-lines to G10.6–0.4 (W31C), W49N, and W51 |
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Interstellar H2 - The population of excited rotational states and the infrared response to ultraviolet radiation |
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Interstellar molecules in the Large Magellanic Cloud |
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Interstellar O2. I. Abundance, excitation, and prospects for detection of 16O18O at radio frequencies |
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Interstellar O2. II. VUV oscillator strengths of Schumann-Runge linesand prospects for space telescope observations |
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Investigating the nature of the Fried Egg nebula |
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ISO-SWS observations of pure rotational H_2_O absorption lines toward Orion-IRc2 |
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Large 12CO/13CO intensity ratios in luminous mergers |
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Low upper limits on the O_2_ abundance from the Odin satellite |
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Millimetre observations of southern translucent clouds |
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Modèle des fronts de photoevaporation dans les régions de formation d'étoiles |
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Molecular gas and dust in the highly magnifiedz ~ 2.8 galaxy behind the Bullet Cluster |
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Molecular gas associated with the ejecta ring nebula around the Wolf-Rayet star WR 16 |
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Molecular gas in starburst galaxies: line intensities and physical conditions |
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Molecular oxygen in the ρ Ophiuchi cloud |
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Molecules at early epochs. IV. Confirmation of the detection of H2 toward PKS 0528-250 |
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Molecules at early epochs. VI. A search for molecular hydrogen in the z = 3.391 damped Lyman alpha system toward Q 0000-263 |
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Molecules at high redshift. V. Improved limits on the column density of CO in two damped Lyman-alpha absorption systems |
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Molecules atz= 0.89 |
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Molecules in planetary nebulae |
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Multi-line detection of O2towardρOphiuchi A |
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Near-infrared observations of the proto-planetary nebula AFGL 618 |
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Nitrogen hydrides in interstellar gas |
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An observational determination of the proton to electron mass ratio in the early universe |
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Observational study of reactive ions and radicals in PDRs |
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Odin observations of H_2_O in the Galactic Centre |
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Odin water mapping in the Orion KL region |
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OH+and H2O+absorption toward PKS 1830–211 |
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On the accretion process in a high-mass star forming region. A multitransitional THz Herschel-HIFI study of ammonia toward G34.26+0.15 |
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An optical ultrahigh-resolution cross-dispersed echelle spectrograph with adaptive optics |
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Optically observed upper limits at z = 1.776 on CO and predictions for the detection of H2 with space telescope |
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Ortho-to-para ratio of NH_2_. Herschel-HIFI observations of ortho- and para-NH_2_ rotational transitions towards W31C, W49N, W51, and G34.3+0.1 |
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Oscillator strengths and ground-state photoionization cross-sections for Mg+ and Ca+ |
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Oscillator strengths for lines of the (0,0) and (1,0) bands of the C1PI-X1 SIG+ system of HCl and the abundance of HCl in diffuse interstellar clouds |
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P Cygni profiles of molecular lines toward Arp 220 nuclei |
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PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars |
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Peculiar molecular clouds in NGC 3256 ? |
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The perplexing spectrum of AFGL 2789 (V645 Cygni) |
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The photodissociation and chemistry of interstellar CO |
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Physical and chemical structure of the IC 63 nebula. II. Chemical models |
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A precise and accurate determination of the cosmic microwave background temperature atz= 0.89 |
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Resolving the shocked gas in HH 54 with Herschel. CO line mapping at high spatial and spectral resolution |
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Rotational fine-structure lines of interstellar C2 toward zeta Persei |
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A search for emission from vibrationally excited H2 |
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Simultaneous ultraviolet, optical and X-ray observations of the X-ray source Vela X-1 (HD 77581) |
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Solar Science with the Atacama Large Millimeter/Submillimeter Array—A New View of Our Sun |
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Spatially extended OH^+^ emission from the Orion Bar and Ridge |
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Spatially resolved images of reactive ions in the Orion Bar,★★. |
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A spectral line survey of Orion KL in the bands 486-492 and 541-577 GHz with the Odin satellite. II. Data analysis |
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Spectroscopy of PKS 0528-250: new limits on CO absorption and emission |
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The spectrum of magnesium hydride |
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SSALMON – The Solar Simulations for the Atacama Large Millimeter Observatory Network |
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The structure of the high-latitude molecular cloud toward HD 210121 |
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Submillimeter wavelength observations of CS towards the core of M17 |
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Sulphur molecules in the circumstellar envelopes of M-type AGB stars |
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Tentative detection of CO^+^ toward Cygnus A |
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Theoretical studies of diffuse cloud chemistry |
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Tracing the sources of cosmic rays with molecular ions |
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The translucent molecular clouds toward HD 154368. I. Extinction, abundances, and depletions |
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Ubiquitous argonium (ArH+) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gas |
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An ultraviolet search for interstellar CS |
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Ultraviolet spectroscopic observations of VV Cephei |
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Unresolved velocity structure in diffuse interstellar clouds |
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Upper limits to interstellar NH+and para-NH2−abundances |
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V645 Cyg - On the structure of a YSO |
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Variations in H 2 O + /H 2 O ratios toward massive star-forming regions |
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VELOCITY-RESOLVED [C ii] EMISSION AND [C ii]/FIR MAPPING ALONG ORION WITH HERSCHEL. |
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Vibrationally excited H2, HCl, and NO+ in the diffuse clouds toward dzeta Ophiuchi |
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Water and ammonia abundances in S140 with the Odin satellite |
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Widespread rotationally hot hydronium ion in the galactic interstellar medium |
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