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ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 02/2015, Volume 800, Issue 1, pp. 1 - 22
Journal Article
Astronomy & astrophysics, ISSN 0004-6361, 09/2018, Volume 616, p. A174
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2017, Volume 467, Issue 3, pp. 3140 - 3159
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 02/2015, Volume 800, Issue 1, p. 1
The [C II] 157.74 μm transition is the dominant coolant of the neutral interstellar gas, and has great potential as a star formation rate (SFR) tracer. Using... 
infrared: galaxies | galaxies: ISM | ISM: structure | galaxies: star formation | LUMINOSITY | CONVERSION | ULTRAVIOLET RADIATION | CORRELATIONS | POTENTIALS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | COLOR | SYNTHESIS | STARS | GALAXIES | EMISSION | BRIGHTNESS | GALAXY NUCLEI | SURFACES
Journal Article
The Astrophysical Journal: an international review of astronomy and astronomical physics, ISSN 0004-637X, 06/2017, Volume 842, Issue 1, p. 4
With its relatively low ionization potential, C+ can be found throughout the interstellar medium (ISM) and provides one of the main cooling channels of the ISM... 
galaxies: ISM
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 471, Issue 3, pp. 3152 - 3185
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 08/2016, Volume 826, Issue 2
The [N II] 122 and 205 pm transitions are powerful tracers of the ionized gas in the interstellar medium. By combining data from 21 galaxies selected from the... 
SUBMILLIMETER GALAXY | PHYSICAL CONDITIONS | FINE-STRUCTURE LINES | STAR-FORMATION RATE | galaxies: star formation | INTERSTELLAR-MEDIUM | ISM: structure | STARBURST GALAXIES | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | RADIATION PRESSURE | HII-REGIONS | COLLISION STRENGTHS | ULTRALUMINOUS INFRARED GALAXIES | Physics - Astrophysics of Galaxies
Journal Article
Publications of the Astronomical Society of the Pacific, ISSN 0004-6280, 03/2010, Volume 122, Issue 889, pp. 261 - 287
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 03/2019, Volume 483, Issue 4, pp. 4968 - 4983
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 3, pp. 3181 - 3209
We analyse the sizes, colour gradients, and resolved stellar mass distributions for 36 massive and passive galaxies in the cluster XMMUJ2235-2557 at z=1.39... 
Galaxies: Fundamental parameters | Galaxies: High-redshift | Galaxy: Evolution | Galaxies: Elliptical and lenticular, cD | Galaxies: Clusters: General | Galaxies: Formation | Physics - Astrophysics of Galaxies
Journal Article
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), ISSN 0004-637X, 2017, Volume 842, Issue 1, p. 4
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2016, Volume 826, Issue 2, p. 175
The [N ii] 122 and 205 μ m transitions are powerful tracers of the ionized gas in the interstellar medium. By combining data from 21 galaxies selected from the... 
galaxies: ISM | ISM: structure | galaxies: star formation | Physics | Astrophysics | CALIBRATION | DISTRIBUTION | ELECTRONS | PHOTONS | CORRELATIONS | RELIABILITY | COMPARATIVE EVALUATIONS | DENSITY | FORECASTING | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | INTERSTELLAR SPACE | STAR EVOLUTION | ELECTRON DENSITY | STARS | GALAXIES | EMISSION | BRIGHTNESS | ELECTRON GAS | COSMIC DUST
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 11/2019, Volume 886, Issue 1
The brightest observed emission line in many star-forming galaxies is the ?m line, making it detectable up to z;?;7. In order to better understand and quantify... 
NEARBY GALAXIES | DUST | PHYSICAL CONDITIONS | SPECTRAL ENERGY-DISTRIBUTIONS | FORMING GALAXIES | SPECTROSCOPY | ASTRONOMY & ASTROPHYSICS | REGIONS | C II EMISSION | INTERSTELLAR-MEDIUM | MICRON LINE DEFICIT
Journal Article