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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
Astronomy and Astrophysics, ISSN 0004-6361, 01/2014, Volume 561, pp. np - np
We study the wavelength dependence of the dust emission as a function of position and environment across the disk of M 33 using Spitzer and Herschel... 
Galaxies individual M 33 | Dust extinction | Galaxies star formation | Galaxies ISM | Spirals | Emissivity | Dust | Metallicity | Local group (astronomy) | Disks | Constants | Astronomy
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2007, Volume 473, Issue 1, pp. 91 - 104
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2009, Volume 493, Issue 2, pp. 453 - 466
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2018, Volume 612, p. A35
Context. Planetary nebulae (PNe) are excellent tracers of stellar populations with low surface brightness, and therefore provide a powerful method to detect... 
Galaxies: individual: M 31 | Galaxies: interactions | Local group | Galaxies: individual: M 33 | Planetary nebulae: general | Substructures | Red giant stars | Broadband | Local group (astronomy) | Luminosity | Planetary nebulae | Image detection | Narrowband | Stellar populations | Filters | Surface brightness | Spiral galaxies | Image filters | Star & galaxy formation | Nebulae | Tracers
Journal Article
Astronomy & astrophysics, ISSN 0004-6361, 07/2010, Volume 518, Issue 4
We present an analysis of the first space-based far-IR-submm observations of M 33, which measure the emission from the cool dust and resolve the giant... 
stars: formation | galaxies: individual: M33 | galaxies: evolution | galaxies: ISM | Local Group | ISM: clouds | GRAPHITE
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2010, Volume 510, Issue 1, p. A64
Aims. In the Local Group spiral galaxy M 33, we investigate the correlation between the star formation rate (SFR) surface density, Sigma(SFR), and the gas... 
Galaxies: spiral | Galaxies: individual: M 33 | Local Group | Galaxies: ISM | NEARBY GALAXIES | NGC-5194 M51A | FORMATION LAW | SPIRAL GALAXIES | GALACTIC DISKS | M33 | GIANT MOLECULAR CLOUDS | FORMING GALAXIES | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | galaxies: individual: M 33 | METALLICITY GRADIENT | galaxies: spiral | SCHMIDT LAW
Journal Article