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The Astrophysical Journal, ISSN 0004-637X, 10/2006, Volume 650, Issue 2 I, pp. 933 - 944
Journal Article
Publications of the Astronomical Society of the Pacific, ISSN 0004-6280, 04/2006, Volume 118, Issue 842, pp. 590 - 610
Journal Article
Nature, ISSN 0028-0836, 2013, Volume 499, Issue 7459, pp. 450 - 453
The under-abundance of very massive galaxies(1,2) in the Universe is frequently attributed to the effect of galactic winds(3-6). Although ionized galactic... 
ORIGIN | OUTFLOWS | M82 | MULTIDISCIPLINARY SCIENCES | MASS FUNCTION | GAS | EMISSION | NGC-253 | FEEDBACK | SUPERWINDS | CHANDRA OBSERVATIONS | Stellar winds | Astrophysics | Star formation | Galaxies | Research | Observations | Properties | Wind | Supernovae | Star & galaxy formation | Stars & galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2015, Volume 452, Issue 4, pp. 3435 - 3450
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2018, Volume 479, Issue 2, pp. 2505 - 2533
We present new L-band ($1\mbox{--}2$ GHz) observations of the nearby spiral galaxy M33 with 80 pc resolution obtained with the Karl G. Jansky Very Large Array.... 
Galaxies: individual: M33 | Galaxies: ISM | ISM: kinematics and dynamics | Radio lines: ISM | Physics - Astrophysics of Galaxies | Galactic Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2015, Volume 452, Issue 4, pp. 3435 - 3435
We present a new algorithm for detecting filamentary structure FILFINDER. The algorithm uses the techniques of mathematical morphology for filament... 
Algorithms | Clouds | Brightness | Filaments | Hough transforms | Striations | Belts | Mathematical morphology
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2015, Volume 452, Issue 4, p. 3435
  We present a new algorithm for detecting filamentary structure FILFINDER. The algorithm uses the techniques of mathematical morphology for filament... 
Dust | Algorithms | Clouds | Correlation analysis | Morphology | Magnetic fields
Journal Article
The Astronomical Journal, ISSN 1538-3881, 06/2019, Volume 158, Issue 1, p. 1
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2018, Volume 480, Issue 3, pp. 3193 - 3194
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2019, Volume 485, Issue 2, pp. 2324 - 2342
We investigate how the spectral properties of atomic (HI) and molecular (H-2) gas, traced by CO(2-1), are related in M33 on 80 pc scales. We find the HI and... 
NEARBY GALAXIES | galaxies: individual: M33 | INTERSTELLAR-MEDIUM | STAR-FORMATION LAW | radio lines: galaxies | ISM: molecules | ISM: molecular | CLOUDS | ASTRONOMY & ASTROPHYSICS | EQUILIBRIUM | GAS | DISK | KINEMATICS | Galactic Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 08/2019, Volume 881, Issue 2, p. 90
We investigate how the properties of Galactic giant molecular clouds (GMCs) and their denser substructures (clumps) correlate with the local star formation... 
FORMATION RATES | FORMATION LAW | INTERSTELLAR-MEDIUM | ISM: structure | DUST | dust, extinction | Galaxy: disk | PERSEUS | SERPENS | ASTRONOMY & ASTROPHYSICS | MASS | ISM: clouds | DENSE GAS | MILKY-WAY | SCHMIDT LAW | Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 09/2004, Volume 612, Issue 1, pp. L29 - L32
We examine the hypothesis that hydrostatic pressure alone determines the ratio of atomic to molecular gas averaged over a particular radius in disk galaxies.... 
NEARBY GALAXIES | SURFACE PHOTOMETRY | NEUTRAL HYDROGEN | H-I | GALACTIC DISKS | ON SPIRAL GALAXIES | STAR-FORMATION | ISM : molecules | CO SURVEY | MASS MODELS | galaxies : ISM | ISM : clouds | ASTRONOMY & ASTROPHYSICS | VIRGO CLUSTER | molecular processes | galaxies : structure
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2018, Volume 480, Issue 1, pp. 893 - 904
In the quest to understand high-mass star formation, it is necessary to understand that from which the high-mass stars will form - dense molecular gas clouds... 
Dust | ISM: clouds | Extinction | Galaxy: disc -Galaxy: structure | Submillimetre: ISM | CORES | submillimetre: ISM | LAW | Galaxy: structure | STAR-FORMATION | INTERSTELLAR-MEDIUM | Galaxy: disc | MODEL | LEAST-SQUARES | DARK CLOUDS | dust, extinction | REMOVAL | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2018, Volume 481, Issue 2, pp. 1862 - 1872
Radiative feedback from massive stars can potentially trigger star formation in the surrounding molecular gas. Inspired by the case of radiatively driven... 
Stars: formation | ISM: jets and outflows | Open clusters and associations: individual: Cyg OB2 | stars: formation | RATES | open clusters and associations: individual: Cyg OB2 | EVOLUTION | CLUSTERS | CLOUDS | ASTRONOMY & ASTROPHYSICS | MILKY-WAY | EMISSION
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2011, Volume 737, Issue 1
We estimate the conversion factor relating CO emission to H-2 mass, alpha(CO), in five Local Group galaxies that span approximately an order of magnitude in... 
ISM: clouds | Local Group | extinction | ISM: molecules | dust | galaxies: ISM | IRREGULAR GALAXIES | TO-GAS RATIO | H-I | INTERSTELLAR-MEDIUM | GALAXY EVOLUTION SAGE | CO SURVEY | SMALL-MAGELLANIC-CLOUD | dust, extinction | GIANT MOLECULAR CLOUDS | GAMMA-RAY EMISSION | SPITZER SURVEY | ASTRONOMY & ASTROPHYSICS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 06/2017, Volume 468, Issue 2, pp. 1769 - 1781
The work of Adamo et al. showed that the mass distributions of young massive stellar clusters were truncated above a maximum-mass scale in the nearby galaxy... 
FORMATION LAW | STELLAR CLUSTERS | DENSE GAS FRACTION | galaxies: individual: M83 | LUMINOSITY FUNCTION | stars: formation | GALAXY M-83 | SCALING RELATIONS | STAR-FORMATION EFFICIENCY | ASTRONOMY & ASTROPHYSICS | GOODNESS-OF-FIT | COSMIC TIME | ISM: clouds | Physics - Astrophysics of Galaxies | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article