https://catalogue-scientifique.canada.ca/record=3908592~S6*frc
The Committee, 1995
The aim of the study was to estimate the number of sea trout spawners entering the Drweca River and evaluate their possibilities of crossing the fish ladders...
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De : Réseau des bibliothèques scientifiques fédérales
https://catalogue-scientifique.canada.ca/record=3908592~S6*frc
The aim of the study was to estimate the number of sea trout spawners entering the Drweca River and evaluate their possibilities of crossing the fish ladders...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=d3ab9bdb-72bd-43f2-88e8-5981a5a3bcfd
Context. The origin of the stellar initial mass function (IMF) and its relation with the core mass function (CMF) are actively debated issues with important...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=5e350b97-be48-4420-a70a-a276f24a9329
We present a catalog of 315 protostellar outflow candidates detected in SiO J = 5 − 4 in the ALMA-IMF Large Program, observed with ∼2000 au spatial resolution,...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=4b5ab9e4-45b5-4216-8c03-0d7ed07ae0d9
ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=d771b161-2351-4495-a1ef-d81486373fb3
The Herschel Gould Belt survey mapped the nearby (d < 500 pc) star-forming regions to understand better how the prestellar phase influences the star formation...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=33dd5152-e133-4170-a323-fa94eeaf8f47
We present a detailed study of the Orion B molecular cloud complex (d ~ 400 pc), which was imaged with the PACS and SPIRE photometric cameras at wavelengths...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=b27fa3f4-d447-4329-97bf-ea285e5c6a2a
We present the first data release of the ALMA-IMF Large Program, which covers the 12m-array continuum calibration and imaging. The ALMA-IMF Large Program is a...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=5ded2741-ae0c-4644-a095-803fd55ad8e5
Aims. Thanks to the high angular resolution, sensitivity, image fidelity, and frequency coverage of ALMA, we aim to improve our understanding of star...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=902138f6-a361-472b-a7a1-9cf7271c65fe
We present far-infrared observations of Monoceros R2 (a giant molecular cloud at approximately 830 pc distance, containing several sites of active star...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=69d6be29-d26e-4af1-83ba-15cbd1f03911
Aims. To constrain models of high-mass star formation, the Herschel-HOBYS key program aims at discovering massive dense cores (MDCs) able to host the high-mass...
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