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Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core mass function
(EDP Sciences, 2015)
A complete understanding of the origin of the prestellar core mass function (CMF) is crucial. Two major features of the prestellar CMF are 1) a broad peak below 1M(circle dot), presumably corresponding to a mean gravitational ...
ALMA 1.3 mm map of the HD 95086 system
(IOP Publishing Ltd., 2017)
Planets and minor bodies such as asteroids, Kuiper-Belt objects, and comets are integral components of a planetary system. Interactions among them leave clues about the formation process of a planetary system. The signature ...
Massive star formation in the GMC G345.5+1.0: spatial distribution of the dust emission
(2011)
Context. Massive condensations in giant molecular clouds (GMCs) are linked to the formation of high mass stars, which are the principal source of heavy elements and UV radiation, playing an important role in the evolution ...
Massive star formation in the GMC G345.5+1.0: spatial distribution of the dust emission
(EDP SCIENCES S A, 2011-10)
Context. Massive condensations in giant molecular clouds (GMCs) are linked to the formation of high mass stars, which are the principal source of heavy elements and UV radiation, playing an important role in the evolution ...
From Peculiar Morphologies to Hubble–type Spirals: The relation between galaxy dynamics and morphology in star–forming galaxies at z ∼ 1.5
(Royal Astronomical Society, 2020)
We present an analysis of the gas dynamics of star-forming galaxies at z ∼ 1.5 using data from the KMOS Galaxy Evolution Survey. We quantify the morphology of the galaxies using HSTCANDELS imaging parametrically and ...
Vales. VII. Molecular and ionized gas properties in the pressure balanced interstellar medium of starburst galaxies at z similar to 0.15
(EDP Sciences, 2020)
Context. Spatially resolved observations of the ionized and molecular gas are critical for understanding the physical processes that govern the interstellar medium (ISM) in galaxies. The observation of starburst systems ...
Probing the anomalous extinction of four young star clusters: the use of colour-excess, main-sequence fitting and fractal analysis
(EDP SCIENCES S ALES ULIS CEDEX A, 2012)
Aims. We studied four young star clusters to characterise their anomalous extinction or variable reddening and asses whether they could be due to contamination by either dense clouds or circumstellar effects. Methods. We ...
Chemical evolution models for spiral disks: the Milky Way, M31, and M33
(EDP SCIENCES S A, 2010)
Context. The distribution of chemical abundances and their variation with time are important tools for understanding the chemical evolution of galaxies. In particular, the study of chemical evolution models can improve our ...