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The Astrophysical journal, ISSN 1538-4357, 10/2019, Volume 884, Issue 1, p. 6
The star-forming region of the Orion Nebula (ONC) is ideal to study the stellar dynamics of young stars in a clustered environment... 
Physical Sciences | Astronomy & Astrophysics | Science & Technology | Space telescopes | Dynamic tests | Orion nebula | Pre-main sequence stars | Star formation | Ejection
Journal Article
The Astrophysical journal, ISSN 0004-637X, 03/2017, Volume 837, Issue 2, p. 151
The common assumption that theta(1) Ori C is the dominant ionizing source for the Orion Nebula is critically examined... 
Ori C, θ | Ori A | H II regions | ISM: individual objects (Orion Nebula) | stars: individual (θ | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Ionization | Orion nebula
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2018, Volume 478, Issue 1, pp. 1017 - 1041
The existence of multiple layers in the inner Orion nebula has been revealed using data from an Atlas of spectra at 2 arcsec and 12 km s(-1) resolution... 
ISM: individual objects: Orion nebula (NGC 1976) | ISM: atoms | Dust, extinction -HII regions | Atomic processes | Radiation mechanisms: general | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Astrophysics of Galaxies
Journal Article
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 2016, Volume 463, Issue 3, pp. 2864 - 2884
In order to study the nature, origin, and impact of turbulent velocity fluctuations in the ionized gas of the Orion nebula, we apply a variety of statistical techniques to observed velocity cubes... 
Hydrodynamics | Turbulence | H ii regions | ISM: kinematics and dynamics | ISM: individual objects: m 42 | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Evaporation | Nebulae | Velocity | Dispersion | Turbulent flow | Fluid dynamics | Ionization | Filaments | Fluctuation | Orion nebula | Physics - Astrophysics of Galaxies
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2018, Volume 478, Issue 2, pp. 1825 - 1836
We present a survey for the tightest visual binaries among 0.3-2M(circle dot) members of the Orion nebula Cluster (ONC... 
Binaries: visual | Open clusters and associations: individual: Orion Nebula Cluster | Stars: pre-main-sequence | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics | Astrophysics
Journal Article
Annual review of astronomy and astrophysics, ISSN 0066-4146, 09/2001, Volume 39, Issue 1, pp. 99 - 136
The Orion Nebula (M 42) is one of the best studied objects in the sky. The advent of multi-wavelength investigations and quantitative high resolution imaging... 
star formation | protoplanetary disks | gaseous nebulae | stellar evolution | Gaseous nebulae | Stellar evolution | Protoplanetary disks | Star formation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Astronomical research | Research | Observations | Nebulae | Stars | Orion Nebula
Journal Article