Listar por tema "ISM: clouds"
Mostrando ítems 1-5 de 5
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Article
Completing the protostellar luminosity function in Cygnus-X with SOFIA/FORCAST imaging (2022)
(Oxford University Press, 2022-05-01)We present a new SOFIA/FORCAST mid-infrared survey of luminous protostars and crowded star-forming environments in Cygnus X, the nearest million-solar mass molecular cloud complex. We derive bolometric luminosities for ... -
Article
Density distributions, magnetic field structures, and fragmentation in high-mass star formation (2024)
(EDP Sciences, 2024)Context. The fragmentation of high-mass star-forming regions depends on a variety of physical parameters, including density, the magnetic field, and turbulent gas properties. Aims. We evaluate the importance of the density ... -
Article
Pillars of Creation among Destruction: Star Formation in Molecular Clouds near R136 in 30 Doradus (2020)
(Institute of Physics Publishing, 2018) -
Article
Resolved observations at 31 GHz of spinning dust emissivity variations in ρ Oph (2020)
(Oxford University Press, 2020-05-14)The ρ Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the cosmic background imager (CBI). Here, we present 4.5 arcmin observations with CBI 2 that confirm 31 GHz emission from ... -
Article
Resolved spectral variations of the centimetre-wavelength continuum from the ρ Oph W photodissociation (2021)
(Oxford University Press, 2021-03-01)Centimetre-wavelength radio continuum emission in excess of free-free, synchrotron, and Rayleigh-Jeans dust emission (excess microwave emission, EME), and often called 'anomalous microwave emission', is bright in molecular ...