https://catalogue-scientifique.canada.ca/record=1307795~S6*frc
Rechercher Lindman, Björn; Rechercher Olofsson, G; Rechercher Stenius, Per; Rechercher Aniansson, Gunnar; Rechercher Stenius, P
Steinkopff, 1985
Actes de conférence
De : Réseau des bibliothèques scientifiques fédérales
https://catalogue-scientifique.canada.ca/record=1307795~S6*frc
https://publications-cnrc.canada.ca/fra/voir/objet/?id=ca4c9226-a38b-44e5-a842-022a3c8fa0e6
Molecular gas constitutes the dominant mass component of protoplanetary discs. To date, these sources have not been studied comprehensively at the longest...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=78ce62ec-668d-46f9-8d5a-fe75c1743310
The young star β Pictoris is well known for its dusty debris disk produced through collisional grinding of planetesimals, kilometre-sized bodies in orbit...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=897b0759-ac29-4713-b142-27139bc82e6e
Τ Ceti is a nearby, mature G-type star very similar to our Sun, with a massive Kuiper Belt analogue and possible multiplanet system that has been compared to...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=15bc7ea2-d010-4743-95aa-6d0562396fc4
Herschel images in six photometric bands show the thermal emission of the debris disk surrounding β Pic. In the three PACS bands at 70 μm, 100 μm and 160 μm...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=0b5ca8b6-410f-422e-b031-10818e143e9b
Context. Stars form surrounded by gas-and dust-rich protoplanetary discs. Generally, these discs dissipate over a few (3-10) Myr, leaving a faint tenuous...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=237b7418-d46a-4a17-901c-ca754f08d506
Some planetary systems harbour debris disks containing planetesimals such as asteroids and comets. Collisions between such bodies produce small dust particles,...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=19dd5a04-660f-430b-a95d-8c13b92cc800
Far-infrared Herschel images of the ε Eridani system, seen at a fifth of the Sun's present age, resolve two belts of debris emission. Fits to the 160 μm PACS...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=3f4de3dc-3d95-4d2e-805d-f1428687855f
Many nearby main-sequence stars have been searched for debris using the far-infrared Herschel satellite, within the DEBRIS, DUNES and Guaranteed-Time Key...
https://publications-cnrc.canada.ca/fra/voir/objet/?id=0e655a0e-03f6-45f5-aba3-4e2b9d6b084a
Context. Fomalhaut is a young (2 ± 1 × 10^8 years), nearby (7.7 pc), 2 M⊙ star that is suspected to harbor an infant planetary system, interspersed with one or...
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