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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 10/2015, Volume 582, pp. A1 - 33
Aims. Our goal is to identify bipolar H II regions and to understand their morphology, their evolution, and the role they play in the formation of new generations of stars. Methods... 
00.14 | ISM: individual objects: G010.32 | Stars: formation | HII regions | ISM: individual objects: G319.88+00.79 | Dust, extinction | Physical Sciences | Astronomy & Astrophysics | Science & Technology | H II regions | Molecular structure | Clouds | Searching | Morphology | Formations | Estimates | Density | Physics | Astrophysics
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2013, Volume 435, Issue 1, pp. 400 - 428
We present a complete sample of molecular clumps containing compact and ultracompact H ii (UC H ii) regions between = 10° and 60° and |b| < 1... 
ISM: HII regions | ISM: clouds | Galaxy: structure | Radio continuum: ISM | Stars: early-type | Stars: formation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Luminosity | Star & galaxy formation | Ultraviolet astronomy | Kinematics | Methanol | Sciences of the Universe | Astrophysics
Journal Article
The Astrophysical journal, ISSN 0004-637X, 10/2009, Volume 703, Issue 2, pp. 1352 - 1362
We evaluate the role of radiation pressure in the dynamics of H II regions. We first determine under what conditions radiation pressure is significant... 
Stars: Winds, outflows | Hii regions | Radiative transfer | Galaxies: Star clusters | Stars: formation | ISM: Bubbles | RADIANT HEAT TRANSFER | STAR CLUSTERS | MATHEMATICAL SOLUTIONS | ENERGY TRANSFER | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STARS | EVALUATION | HEAT TRANSFER | GALAXIES | COMPARATIVE EVALUATIONS | RADIATION PRESSURE
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 01/2015, Volume 573
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 01/2017, Volume 597, p. A84
.... This work aims to determine accurately the physical and chemical properties of a sample of HII regions located at R-G... 
Galaxy: evolution | Hii regions | Galaxy: disk | Galaxy: abundances | ISM: abundances | Physical Sciences | Astronomy & Astrophysics | Science & Technology
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2013, Volume 553, pp. 1 - 11
Aims. We systematically study the relations between the H alpha luminosity and the near-IR luminosity and temperature of a set of selected HII regions in the disc of M100. Methods... 
Infrared: ISM | Methods: statistical | HII regions | Galaxies: ISM | Galaxies: individual: M 100 | Infrared: galaxies | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Band spectra | Fittings | Dust | Images | Emission | Luminosity | Color temperature | Colour
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2013, Volume 428, Issue 3, pp. 1927 - 1943
...) in their host galaxies have variously claimed an association with HII regions; no association; or an association only with hydrogen-deficient ccSNe... 
Supernovae: general | HII regions | Galaxies: ISM | Stars: massive | Physics - Solar and Stellar Astrophysics
Journal Article
The Astronomical journal, ISSN 1538-3881, 10/2011, Volume 142, Issue 4, pp. 139 - jQuery1323897164051='48'
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2018, Volume 479, Issue 3, pp. 3264 - 3273
Measurements of the galaxy UV luminosity function at z greater than or similar to 6 suggest that young stars hosted in low-mass star-forming galaxies produced... 
First stars | Galaxies: evolution | Dark ages | Galaxies: ism | Reionization | H ii regions | Methods: data analysis | Galaxies: dwarf | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Astrophysics of Galaxies | Cosmology and Extra-Galactic Astrophysics | Physics | Astrophysics
Journal Article