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1. Full Text The 21-SPONGE H i Absorption Line Survey. I. The Temperature of Galactic H i
by Murray, Claire E and Stanimirović, Snežana and Goss, W.M and Heiles, Carl and Dickey, John M and Babler, Brian and Kim, Chang-Goo
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 10/2018, Volume 238, Issue 2, p. 14
radio lines: ISM | ISM: clouds | ISM: structure
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2. Full Text The Leiden/Argentine/Bonn (LAB) survey of Galactic HI: Final data release of the combined IDS and IAR surveys with improved stray-radiation corrections
by Kalberla, P.M.W and Burton, W.B and Hartmann, Dap and Arnal, E.M and Bajaja, E and Morras, R and Pöppel, W.G.L
Astronomy and Astrophysics, ISSN 0004-6361, 09/2005, Volume 440, Issue 2, pp. 775 - 782
Surveys | Galaxy: structure | Radio lines: ISM
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3. Full Text An ALMA Survey of DCN/H13CN and DCO+/H13CO+ in Protoplanetary Disks
by Huang, Jane and Oberg, Karin I and Qi, Chunhua and Aikawa, Yuri and Andrews, Sean M and Furuya, Kenji and Guzmán, Viviana V and Loomis, Ryan A and Van Dishoeck, Ewine F and Wilner, David J
Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 835, Issue 2, p. 231
protoplanetary disks | radio lines: ISM | ISM: molecules | astrochemistry
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4. Full Text The CO-to-H 2 conversion factor
by Bolatto, Alberto D and Wolfire, Mark and Leroy, Adam K
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 08/2013, Volume 51, pp. 207 - 268
CO line emission represents the most accessible and widely used tracer of the molecular ISM. This renders the translation of observed CO intensity into total... 
ISM: general | ISM: molecules | Galaxies: ISM | Radio lines: ISM | HIGH-RESOLUTION CO | DIFFUSE INTERSTELLAR-MEDIUM | LUMINOUS INFRARED GALAXIES | STAR-FORMATION RATE | HIGH-REDSHIFT GALAXIES | SMALL-MAGELLANIC-CLOUD | GIANT MOLECULAR CLOUDS | radio lines: ISM | GAMMA-RAY EMISSION | galaxies: ISM | SEST KEY PROGRAM | ASTRONOMY & ASTROPHYSICS | TRANSLUCENT SIGHT LINES
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5. Full Text Large-Scale Structure of the Molecular Gas in Taurus Revealed by High Linear Dynamic Range Spectral Line Mapping
by Goldsmith, Paul F and Heyer, Mark and Narayanan, Gopal and Snell, Ronald and Li, Di and Brunt, Chris
The Astrophysical Journal, ISSN 0004-637X, 06/2008, Volume 680, Issue 1, pp. 428 - 445
We report the results of a 100 deg(2) survey of the Taurus molecular cloud region in (CO)-C-12 and (CO)-C-13 J = 1 -> 0. The image of the cloud in each... 
ISM: individual (Taurus) | ISM: evolution | ISM: molecules | Stars: formation | Radio lines: ISM | ISM : individual (Taurus) | STAR-FORMATION | RATIO | ISM : molecules | radio lines : ISM | INTERSTELLAR-MEDIUM | CARBON-MONOXIDE ABUNDANCE | NARROW SELF-ABSORPTION | (CO)-O-18 SURVEY | DARK CLOUDS | DENSE CLOUD CORES | T-TAURI | stars : formation | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | ISM : evolution | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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6. Full Text An ammonia spectral map of the L1495-B218 filaments in the taurus molecular cloud. II. CCS and HC 7 N chemistry and three modes of star formation in the filaments
by Seo, Young Min and Majumdar, Liton and Goldsmith, Paul F and Shirley, Yancy L and Willacy, Karen and Ward-Thompson, Derek and Friesen, Rachel and Frayer, David and Church, Sarah E and Chung, Dongwoo and Cleary, Kieran and Cunningham, Nichol and Devaraj, Kiruthika and Egan, Dennis and Gaier, Todd and Gawande, Rohit and Gundersen, Joshua O and Harris, Andrew I and Kangaslahti, Pekka and Readhead, Anthony C. S and Samoska, Lorene and Sieth, Matthew and Stennes, Michael and Voll, Patricia and White, Steve
Astrophysical Journal, ISSN 0004-637X, 02/2019, Volume 871, Issue 2
surveys | radio lines: ISM | ISM: Clouds | ISM: Molecules | stars: Formation
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7. Full Text Dense cores in Perseus: The influence of stellar content and cluster environmen
by Foster, Jonathan B and Rosolowsky, Erik W and Kauffmann, Jens and Pineda, Jaime E and Borkin, Michelle A and Caselli, Paola and Myers, Phil C and Goodman, Alyssa A
Astrophysical Journal, ISSN 0004-637X, 05/2009, Volume 696, Issue 1, pp. 298 - 319
ISM: molecules | ISM: clouds | Radio lines: ISM
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8. Full Text Deuterium and 15N fractionation in N2H+ during the formation of a Sun-like star
by De Simone, M and Fontani, F and Codella, C and Ceccarelli, C and Lefloch, B and Bachiller, R and López-Sepulcre, A and Caux, E and Vastel, C and Soldateschi, J
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2018, Volume 476, Issue 2, pp. 1982 - 1990
ISM: clouds | ISM: molecules | Stars: formation | Radio lines: ISM
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9. Full Text Squeezed between shells? the origin of the Lupus i molecular cloud: II. APEX CO and GASS H i observations
by Gaczkowski, B and Roccatagliata, V and Flaischlen, S and Kröll, D and Krause, M.G.H and Burkert, A and Diehl, R and Fierlinger, K and Ngoumou, J and Preibisch, T
Astronomy and Astrophysics, ISSN 0004-6361, 12/2017, Volume 608, p. A102
ISM: clouds | ISM: molecules | ISM: bubbles | ISM: structure | ISM: kinematics and dynamics | Radio lines: ISM
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10. Full Text The radial distribution of H2 and co in tw hya as revealed by resolved alma observations of co isotopologues
by Schwarz, Kamber R and Bergin, Edwin A and Cleeves, L. Ilsedore and Blake, Geoffrey A and Zhang, Ke and Öberg, Karin I and Van Dishoeck, Ewine F and Qi, Chunhua
Astrophysical Journal, ISSN 0004-637X, 06/2016, Volume 823, Issue 2
CO is widely used as a tracer of molecular gas. However, there is now mounting evidence that gas phase carbon is depleted in the disk around TW Hya. Previous... 
protoplanetary disks | molecular data | radio lines: ISM | astrochemistry | circumstellar matter | ISM: abundances
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11. Full Text A computer program for fast non-LTE analysis of interstellar line spectra - With diagnostic plots to interpret observed line intensity ratios
by van der Tak, F. F. S and Black, J. H and Schoeier, F. L and Jansen, D. J and van Dishoeck, E. F
Astronomy & astrophysics, ISSN 0004-6361, 06/2007, Volume 468, Issue 2, pp. 627 - U261
Aims. The large quantity and high quality of modern radio and infrared line observations require efficient modeling techniques to infer physical and chemical... 
Infrared: ISM | Radiative transfer | Submillimeter | Methods: numerical | Radio lines: ISM | PHYSICAL CONDITIONS | MOLECULAR CLOUDS | radiative transfer | IRAS 16293-2422 | radio lines : ISM | infrared : ISM | RADIATIVE-TRANSFER | submillimeter | MASSIVE YOUNG STARS | CHEMICAL VARIATIONS | OH MASERS | MODELS | CARBON-MONOXIDE | ASTRONOMY & ASTROPHYSICS | methods : numerical | STAR-FORMING REGION
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12. Full Text A sensitive λ 3 mm line survey of L483: A broad view of the chemical composition of a core around a Class 0 object
by Agúndez, M and Marcelino, N and Cernicharo, J and Roueff, E and Tafalla, M
Astronomy and astrophysics, ISSN 0004-6361, 07/2019, Volume 625, p. A147
An exhaustive chemical characterization of dense cores is mandatory to our understanding of chemical composition changes from a starless to a protostellar... 
ISM: clouds | line: identification | radio lines: ISM | ISM: molecules | astrochemistry
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13. Full Text Seeds of Life in Space (SOLIS): The Organic Composition Diversity at 300-1000 au Scale in Solar-type Star-forming Regions
by Ceccarelli, C and Caselli, P and Fontani, F and Neri, R and López-Sepulcre, A and Codella, C and Feng, S and Jiménez-Serra, I and Lefloch, B and Pineda, J.E and Vastel, C and Alves, F and Bachiller, R and Balucani, N and Bianchi, E and Bizzocchi, L and Bottinelli, S and Caux, E and Chacón-Tanarro, A and Choudhury, R and Coutens, A and Dulieu, F and Favre, C and Hily-Blant, P and Holdship, J and Kahane, C and Al-Edhari, A. Jaber and Laas, J and Ospina, J and Oya, Y and Podio, L and Pon, A and Punanova, A and Quenard, D and Rimola, A and Sakai, N and Sims, I.R and Spezzano, S and Taquet, V and Testi, L and Theulé, P and Ugliengo, P and Vasyunin, A.I and Viti, S and Wiesenfeld, L and Yamamoto, S
Astrophysical Journal, ISSN 0004-637X, 12/2017, Volume 850, Issue 2, p. 176
Complex organic molecules have been observed for decades in the interstellar medium. Some of them might be considered as small bricks of the macromolecules at... 
ISM: clouds | radio lines: ISM | ISM: molecules | ISM: abundances | SPITZER C2D SURVEY | COMPLEX-MOLECULES | HOT CORE | MILLIMETER-WAVE | GAS-PHASE FORMATION | NEARBY DENSE CORES | MASS PROTOSTAR IRAS-16293-2422 | HARO ENERGY-SOURCES | MICROWAVE-SPECTRA | ASTRONOMY & ASTROPHYSICS | MOLECULAR-SPECTROSCOPY | Physics | Astrophysics
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14. Full Text High-accuracy quartic force field calculations for the spectroscopic constants and vibrational frequencies of 11 A′ l-C 3H-: A possible link to lines observed in the horsehead nebula photodissociation region
by Fortenberry, Ryan C and Huang, Xinchuan and Crawford, T. Daniel and Lee, Timothy J
Astrophysical Journal, ISSN 0004-637X, 07/2013, Volume 772, Issue 1
ISM: lines and bands | molecular data | radio lines: ISM | ISM: molecules | astrochemistry | ISM: individual objects (Horsehead nebula)
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15. Full Text Detection of 15NH2 D in dense cores: A new tool for measuring the 14N/15N ratio in the cold ISM
by Gerin, M and Marcelino, N and Biver, N and Roueff, E and Coudert, L.H and Elkeurti, M and Lis, D.C and Bockelée-Morvan, D
Astronomy and Astrophysics, ISSN 0004-6361, 05/2009, Volume 498, Issue 2, pp. L9 - L12
Astrochemistry | ISM: clouds | ISM: general | ISM: molecules | Radio lines: ISM
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16. Full Text ALMA spectral survey of Supernova 1987A - molecular inventory, chemistry, dynamics and explosive nucleosynthesis
by Matsuura, M and Indebetouw, R and Woosley, S and Bujarrabal, V and Abellán, F.J and McCray, R and Kamenetzky, J and Fransson, C and Barlow, M.J and Gomez, H.L and Cigan, P and De Looze, I and Spyromilio, J and Staveley-Smith, L and Zanardo, G and Roche, P and Larsson, J and Viti, S and van Loon, J. Th and Wheeler, J.C and Baes, M and Chevalier, R and Lundqvist, P and Marcaide, J.M and Dwek, E and Meixner, M and Ng, C.-Y and Sonneborn, G and Yates, J and Naturvetenskapliga fakulteten and Institutionen för astronomi and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2017, Volume 469, Issue 3, pp. 3347 - 3362
We report the first molecular line survey of Supernova 1987A in the millimetre wavelength range. In the Atacama Large Millimeter/submillimeter Array (ALMA)... 
Supernovae: individual: Supernova 1987A | ISM: supernova remnants | ISM: molecules | ISM: abundances | Radio lines: ISM | supernovae: individual: Supernova 1987A | MASSIVE STARS | LINE EMISSION | NEBULA M 1-92 | INFRARED WATER-VAPOR | radio lines: ISM | CARBON-MONOXIDE | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | SN 1987A | LARGE-MAGELLANIC-CLOUD | CIRCUMSTELLAR RING | II-P SUPERNOVAE | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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