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1. Full Text The molecular gas in luminous infrared galaxies - I. CO lines, extreme physical conditions and their drivers
by Papadopoulos, Padelis P and van der Werf, Paul P and Xilouris, E. M and Isaak, K. G and Gao, Yu and Mühle, S
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2012, Volume 426, Issue 4, pp. 2601 - 2629
Abstract We report results from a large molecular line survey of luminous infrared galaxies (LIRGs; L IR ≳1011L⊙) in the local Universe (z ≤ 0.1), conducted... 
galaxies: starburst | infrared: galaxies | cosmic rays | radio lines: ISM | ISM: molecules | galaxies: ISM | Galaxies: starburst | Cosmic rays | Galaxies: ISM | Infrared: galaxies | Radio lines: ISM | STAR-FORMING GALAXIES | RAY DOMINATED REGIONS | SEYFERT-GALAXIES | INTERSTELLAR-MEDIUM | STARBURST GALAXIES | ACTIVE GALACTIC NUCLEI | ASTRONOMY & ASTROPHYSICS | DENSE GAS | IRAS GALAXIES | ULTRALUMINOUS GALAXIES | NEARBY SPIRAL GALAXIES | Galaxies | Clouds | Analysis | Luminosity | Cosmology | Stars & galaxies | Astronomy | Infrared | Infrared radiation | Universe | Carbon monoxide | Excitation | Sleds | Physics - Cosmology and Nongalactic Astrophysics
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2. Full Text THE MOLECULAR GAS IN LUMINOUS INFRARED GALAXIES. II. EXTREME PHYSICAL CONDITIONS AND THEIR EFFECTS ON THE X-co FACTOR
by Papadopoulos, PP and van der Werf, P and Xilouris, E and Isaak, KG and Gao, Y
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 05/2012, Volume 751, Issue 1
In this work, we conclude the analysis of our CO line survey of luminous infrared galaxies (LIRGs: L-IR greater than or similar to 10(11) L-circle dot) in the... 
NEARBY GALAXIES | galaxies: starburst | STAR-FORMING GALAXIES | ACTIVE GALACTIC NUCLEUS | INTERSTELLAR-MEDIUM | radiation mechanisms: general | SUBMILLIMETER GALAXIES | CONVERSION FACTOR | galaxies: active | ISM: molecules | galaxies: ISM | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | HIGH-RESOLUTION | DENSE GAS | IRAS GALAXIES | ULTRALUMINOUS GALAXIES
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3. Full Text Black hole mass measurement using molecular gas kinematics: what ALMA can do
by Yoon, I
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711), ISSN 0035-8711, 2017, Volume 466, Issue 2, pp. 1987 - 2005
We study the limits of the spatial and velocity resolution of radio interferometry to infer the mass of supermassive black holes (SMBHs) in galactic centres... 
LUMINOSITY | methods: observational | VELOCITY DISPERSION | ATLAS(3D) PROJECT | HOST GALAXIES | AGN | BULGELESS GALAXIES | EARLY-TYPE GALAXIES | black hole physics | ASTRONOMY & ASTROPHYSICS | NGC 1097 | ISM: kinematics and dynamics galaxies: nuclei | GALACTIC NUCLEI | DENSE GAS | Physics - Astrophysics of Galaxies
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4. 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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5. Full Text The Relationship between Molecular Gas Tracers and Kennicutt-Schmidt Laws
by Krumholz, Mark R and Thompson, Todd A
The Astrophysical Journal, ISSN 0004-637X, 11/2007, Volume 669, Issue 1, pp. 289 - 298
We provide a model for how Kennicutt-Schmidt (KS) laws, which describe the correlation between star formation rate and gas surface or volume density, depend on... 
ISM: clouds | ISM: molecules | Stars: formation | Galaxies: ISM | Radio lines: ISM | STAR-FORMING GALAXIES | SPIRAL GALAXIES | GALACTIC DISKS | ISM : molecules | radio lines : ISM | INTERSTELLAR-MEDIUM | LUMINOUS GALAXIES | galaxies : ISM | stars : formation | ISM : clouds | HIGH-REDSHIFT | ASTRONOMY & ASTROPHYSICS | DENSE GAS | TURBULENCE | ULTRALUMINOUS INFRARED GALAXIES | 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 MODELING the MOLECULAR GAS in NGC 6240
by Tunnard, R and Greve, T.R and Garcia-Burillo, S and Carpio, J. Graciá and Fuente, A and Tacconi, L and Neri, R and Usero, A
Astrophysical Journal, ISSN 0004-637X, 12/2015, Volume 815, Issue 2, p. 114
We present the first observations of (HCN)-C-13 (1 - 0), (HCO+)-C-13(1- 0), and SiO (2 - 1)in NGC 6240, obtained with the TRAM Plateau de Bure Interferometer.... 
galaxies: ISM | submillimeter: ISM | galaxies: individual (NGC 6240) | STAR-FORMATION | ACTIVE GALACTIC NUCLEUS | VIBRATIONALLY EXCITED HCN | ROTATIONAL-EXCITATION | DENSE INTERSTELLAR CLOUDS | ARP 220 | ASTRONOMY & ASTROPHYSICS | SPECTRAL ENERGY-DISTRIBUTION | ULTRALUMINOUS GALAXIES | INFRARED GALAXY NGC-6240 | HNC LINE EMISSION | Physics - Astrophysics of Galaxies
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7. Full Text The Warm Molecular Gas around the Cloverleaf Quasar
by Bradford, C. M and Aguirre, J. E and Aikin, R and Bock, J. J and Earle, L and Glenn, J and Inami, H and Maloney, P. R and Matsuhara, H and Naylor, B. J and Nguyen, H. T and Zmuidzinas, J
The Astrophysical Journal, ISSN 0004-637X, 11/2009, Volume 705, Issue 1, pp. 112 - 122
We present the first broadband lambda = 1 mm spectrum toward the z = 2.56 Cloverleaf quasar, obtained with Z-Spec, a grating spectrograph on the 10.4 m Caltech... 
Planetary systems: formation | Accretion | Planetary systems: protoplanetary disks | Accretion disks | LINE EMISSION | STAR-FORMATION RATE | MAGNETOHYDRODYNAMIC SHOCK-WAVES | instrumentation: spectrographs | stars: luminosity function, mass function | BROAD-BAND | IRAS F10214+4724 | STARBURST GALAXIES | WATER-VAPOR | ASTRONOMY-SATELLITE | galaxies: ISM | techniques: spectroscopic | ASTRONOMY & ASTROPHYSICS | ISM: clouds | DENSE GAS | INITIAL MASS FUNCTION | LUMINOSITY | X RADIATION | OXYGEN COMPOUNDS | HYDROGEN COMPOUNDS | DUSTS | PHOTONS | BOSONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MASS | PHYSICAL PROPERTIES | OPTICAL PROPERTIES | RADIATIONS | WATER | FREQUENCY RANGE | GHZ RANGE 100-1000 | GHZ RANGE | ELEMENTARY PARTICLES | IONIZING RADIATIONS | COSMIC RADIO SOURCES | QUASARS | MASSLESS PARTICLES | ELECTROMAGNETIC RADIATION | STARS | GALAXIES | EMISSION | SPECTRA
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8. Full Text Major impact from a minor merger The extraordinary hot molecular gas flow in the Eye of the NGC 4194 Medusa galaxy
by Konig, S and Aalto, S and Muller, S and Gallagher, JS and Beswick, RJ and Varenius, E and Jutte, E and Krips, M and Adamo, A and Naturvetenskapliga fakulteten and Institutionen för astronomi and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 07/2018, Volume 615, p. A122
Context. Minor mergers are important processes contributing significantly to how galaxies evolve across the age of the Universe. Their impact on the growth of... 
galaxies: starburst | HCN OBSERVATIONS | PHYSICAL CONDITIONS | EXCITATION | galaxies: individual: NGC 4194 | STAR-FORMING GALAXIES | galaxies: evolution | LUMINOUS INFRARED GALAXIES | ACTIVE GALACTIC NUCLEUS | STARBURST GALAXIES | radio lines: ISM | galaxies: active | ISM: molecules | ASTRONOMY & ASTROPHYSICS | DENSE GAS | ULTRALUMINOUS GALAXIES | EMISSION | Physics - Astrophysics of Galaxies | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
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9. Full Text Molecular gas chemistry in AGN II. High-resolution imaging of SiO emission in NGC 1068: Shocks or XDR?
by García-Burillo, S and Usero, A and Fuente, A and Martín-Pintado, J and Boone, F and Aalto, S and Krips, M and Neri, R and Schinnerer, E and Tacconi, L.J
Astronomy and Astrophysics, ISSN 0004-6361, 09/2010, Volume 519, Issue 1, p. A2
Context. This paper is part of a multi-species survey of line emission from the molecular gas in the circum-nuclear disk (CND) of the Seyfert 2 galaxy NGC... 
Nuclei - Galaxies | ISM - Galaxies | Kinematics and dynamics - Galaxies | ISM | Galaxies | Individual | NGC 1068 - Galaxies | Active - Radio lines | LINE EMISSION | SEYFERT-GALAXIES | STAR-FORMATION | ACTIVE GALACTIC NUCLEUS | galaxies: individual: NGC 1068 | HCN | radio lines: ISM | galaxies: active | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | CENTER REGION | X-RAY | DENSE GAS | galaxies: kinematics and dynamics | galaxies: nuclei | ULTRALUMINOUS INFRARED GALAXIES | NGC-1068
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10. Full Text Molecular gas heating mechanisms, and star formation feedback in Merger/Starbursts: NGC 6240 and Arp 193 AS case studies
by Papadopoulos, Padelis P and Zhang, Zhi-Yu and Xilouris, E.M and Weiss, Axel and Van Der Werf, Paul and Israel, F.P and Greve, T.R and Isaak, Kate G and Gao, Y
Astrophysical Journal, ISSN 0004-637X, 06/2014, Volume 788, Issue 2, pp. 153 - 20
We used the SPIRE/FTS instrument aboard the Herschel Space Observatory to obtain the Spectral Line Energy Distributions (SLEDs) of CO from J= 4-3 to J= 13-12... 
galaxies: starburst | galaxies: active | ISM: molecules | galaxies: ISM | techniques: spectroscopic | ISM: abundances | ISM: kinematics and Dynamics | DENSE | INITIAL CONDITIONS | PHYSICAL CONDITIONS | LUMINOUS INFRARED GALAXIES | STARBURSTS | ISM: kinematics and dynamics | INTERSTELLAR-MEDIUM | PHOTODISSOCIATION REGIONS | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER | HERSCHEL-SPIRE | Star formation | Infrared | Galaxies | Gas heating | Space telescopes | Spires | Cobalt | Sleds | EXCITATION | CARBON 13 | DUSTS | PHOTONS | ENERGY SPECTRA | GALACTIC EVOLUTION | CARBON MONOXIDE | ABUNDANCE | MOLECULES | SPACE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | METALS | MASS | STARS | GALAXIES | EFFICIENCY | UNIVERSE | FEEDBACK
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11. Full Text REVEALING THE PHYSICAL PROPERTIES OF MOLECULAR GAS IN ORION WITH A LARGE-SCALE SURVEY IN J=2-1 LINES OF (CO)-C-12, (CO)-C-13, AND (CO)-O-18
by Nishimura, A and Tokuda, K and Kimura, K and Muraoka, K and Maezawa, H and Ogawa, H and Dobashi, K and Shimoikura, T and Mizuno, A and Fukui, Y and Onishi, T
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, ISSN 0067-0049, 01/2015, Volume 216, Issue 1
We present fully sampled similar to 3' resolution images of (CO)-C-12(J = 2-1), (CO)-C-13(J = 2-1), and (CO)-O-18(J = 2-1) emission taken with the newly... 
GOULD BELT | STAR-FORMATION | CO SURVEY | DARK CLOUD | stars: formation | JCMT LEGACY SURVEY | radio lines: ISM | CARBON-MONOXIDE | ASTRONOMY & ASTROPHYSICS | DENSE CORES | ISM: individual objects (Orion) | GALACTIC-CENTER | ISM: clouds | CLOUD-CLOUD COLLISION | MILKY-WAY
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12. Full Text Molecular Gas in Extreme Star-Forming Environments: The Starbursts Arp 220 and NGC 6240 as Case Studies
by Greve, T. R and Papadopoulos, P. P and Gao, Y and Radford, S. J. E
The Astrophysical Journal, ISSN 0004-637X, 02/2009, Volume 692, Issue 2, pp. 1432 - 1446
We report single-dish multitransition measurements of the (CO)-C-12, HCN, and HCO+ molecular line emission as well as HNC J = 1-0 and HNCO in the two... 
ISM: molecules | galaxies: starburst | galaxies: individual (Arp 220, NGC 6240) | THERMAL BALANCE | PHYSICAL CONDITIONS | ACTIVE GALACTIC NUCLEUS | INTERSTELLAR-MEDIUM | LUMINOUS GALAXIES | ROTATIONAL-EXCITATION | ASTRONOMY & ASTROPHYSICS | DENSE GAS | SPECTRAL ENERGY-DISTRIBUTION | ULTRALUMINOUS INFRARED GALAXIES | HNC LINE EMISSION
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13. Full Text An Accreting Supermassive Black Hole Irradiating Molecular Gas in NGC 2110
by Rosario, DJ and Togi, A and Burtscher, L and Davies, RI and Shimizu, TT and Lutz, D
ASTROPHYSICAL JOURNAL LETTERS, ISSN 2041-8205, 04/2019, Volume 875, Issue 1, p. L8
The impact of active galactic nuclei (AGNs) on star formation has implications for our understanding of the relationships between supermassive black holes and... 
galaxies: Seyfert | COEVOLUTION | EXCITATION | SEYFERT-GALAXIES | infrared: ISM | H-2 | STAR-FORMATION LAW | FE-II | ISM: molecules | submillimeter: ISM | NUCLEUS | ASTRONOMY & ASTROPHYSICS | molecular processes | DENSE GAS | galaxies: nuclei | EMISSION
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14. Full Text What Lurks in ULIRGs? - Probing the Chemistry and Excitation of Molecular Gas in the Nuclei of Arp 220 and NGC 6240
by Manohar, Swarnima and Scoville, Nick
Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 835, Issue 2, p. 127
We have imaged the dense star-forming regions of Arp 220 and NGC 6240 in the 3 mm band transitions of CO, HCN, HCO+, HNC, and CS at 0.'' 5-0.'' 8 resolution... 
galaxies: individual (Arp 220 and NGC 6240) | galaxies: starburst | EXTRAGALACTIC CS | STAR-FORMATION | ACTIVE GALACTIC NUCLEUS | CLOUD CORES | LUMINOUS GALAXIES | HCN | ASTRONOMY & ASTROPHYSICS | DENSE GAS | EMISSION | ULTRALUMINOUS INFRARED GALAXIES | CHANDRA OBSERVATIONS | X RADIATION | CARBON | EXCITATION | MOLECULAR IONS | RESOLUTION | SENSITIVITY | CARBON MONOXIDE | HYDROCYANIC ACID | ABUNDANCE | DENSITY | HYDROGEN | NUCLEI | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CLOUDS | STARS | GALAXIES
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15. Full Text Molecular gas kinematics and line diagnostics in early-type galaxies: NGC 4710 and NGC 5866
by Topal, Selçuk and Bureau, Martin and Davis, Timothy A and Krips, Melanie and Young, Lisa M and Crocker, Alison F
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2016, Volume 463, Issue 4, pp. 4121 - 4152
We present interferometric observations of CO lines [(CO)-C-12(1-0, 2-1) and (CO)-C-13(1-0, 2-1)] and dense gas tracers [HCN(1-0), HCO+(1-0), HNC(1-0) and... 
Galaxies: elliptical and lenticular | Galaxies: individual: NGC 5866 | ISM: molecules | CD- galaxies: individual: NGC 4710 | Galaxies: ISM | ATLAS(3D) PROJECT | ELLIPTIC GALAXIES | STAR-FORMATION | galaxies: individual: NGC 5866 | ACTIVE GALACTIC NUCLEUS | INFRARED GALAXIES | galaxies: individual: NGC 4710 | INTERSTELLAR CLOUDS | galaxies: elliptical and lenticular, cD | SPATIALLY-RESOLVED CHEMISTRY | CARBON-MONOXIDE | PHOTODISSOCIATION REGIONS | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | DENSE GAS
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16. Full Text The molecular gas content of the Pipe Nebula: I. Direct evidence of outflow-generated turbulence in B59?
by Duarte-Cabral, A and Chrysostomou, A and Peretto, N and Fuller, G.A and Matthews, B and Schieven, G and Davis, G.R
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 543, p. A140
Context. Star forming regions may share many characteristics, but the specific interplay between gravity, magnetic fields, large-scale dynamics, and... 
Stars: protostars | ISM: jets and outflows | ISM: clouds | Stars: formation | ISM: individual objects: B59 | ISM: kinematics and dynamics | EXTINCTION MAPS | stars: protostars | YOUNG STELLAR OBJECTS | stars: formation | DRIVEN TURBULENCE | SUBMILLIMETER SURVEY | CLOUD EVOLUTION | CARBON-MONOXIDE | ASTRONOMY & ASTROPHYSICS | DENSE CORE POPULATION | STAR-FORMATION ACTIVITY | NEAR-INFRARED SURVEY | LINE FORMATION | Physics - Astrophysics of Galaxies | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
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