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Astronomy and Astrophysics, ISSN 0004-6361, 10/2010, Volume 520, Issue 15, p. A107
Does star formation proceed in the same way in large spirals such as the Milky Way and in smaller chemically younger galaxies? Earlier work suggests a more... 
stars: formation | ISM: clouds | Local Group | galaxies: groups: individual: M 33 | galaxies: evolution | galaxies: ISM | MAGELLANIC-CLOUD | OUTER GALAXY | METALLICITY | M33 | ISOLATED SPIRAL GALAXY | CARBON-MONOXIDE | ASTRONOMY & ASTROPHYSICS | GAS | (CO)-C-13 | EMISSION | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 548, p. A52
Journal Article
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2013, Volume 435, Issue 2, pp. 1598 - 1609
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2016, Volume 593, p. A21
Journal Article
Astronomy & astrophysics, ISSN 0004-6361, 07/2010, Volume 518, Issue 3, p. L70
Context. Over the past few years several studies have provided estimates of the SFR (star-formation rate) or the total infrared luminosity from just one... 
FORMATION RATE INDICATORS | NEARBY GALAXIES | CALIBRATION | galaxies: individual: M33 | infrared: galaxies | TOTAL INFRARED LUMINOSITY | galaxies: star formation | SPITZER | DUST | FORMING GALAXIES | PHOTOMETRY | ULTRAVIOLET | galaxies: spiral | EXTINCTION | Galaxies: spiral | Galaxies: star formation | Galaxies: individual: M 33 | Infrared: galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 11/2016, Volume 595, p. A43
Context. The infrared emission (IR) of the interstellar dust has been claimed to be a tracer of the star formation rate. However, the conversion of the IR... 
Infrared: ISM | Galaxies: individual: M 33 | Hiiregions | ISM: bubbles | Galaxies: ISM | Dust, extinction | Galactic Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2009, Volume 493, Issue 2, pp. 453 - 466
Journal Article