The physical state of selected cold clumps
| dc.contributor.author | Parikka A | |
| dc.contributor.author | Juvela M | |
| dc.contributor.author | Pelkonen VM | |
| dc.contributor.author | Malinen J | |
| dc.contributor.author | Harju J | |
| dc.contributor.organization | fi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO| | |
| dc.contributor.organization-code | 2609700 | |
| dc.converis.publication-id | 3369410 | |
| dc.converis.url | https://research.utu.fi/converis/portal/Publication/3369410 | |
| dc.date.accessioned | 2022-10-28T14:10:20Z | |
| dc.date.available | 2022-10-28T14:10:20Z | |
| dc.description.abstract | <p> Conclusions. The results indicate that most cold clumps, even those with dust color temperatures close to 11 K, are not necessarily prestellar.</p> | |
| dc.identifier.jour-issn | 0004-6361 | |
| dc.identifier.olddbid | 186694 | |
| dc.identifier.oldhandle | 10024/169788 | |
| dc.identifier.uri | https://www.utupub.fi/handle/11111/39386 | |
| dc.identifier.urn | URN:NBN:fi-fe2021042715170 | |
| dc.language.iso | en | |
| dc.okm.affiliatedauthor | Pelkonen, Veli-Matti | |
| dc.okm.discipline | 115 Astronomy and space science | en_GB |
| dc.okm.discipline | 115 Avaruustieteet ja tähtitiede | fi_FI |
| dc.okm.internationalcopublication | international co-publication | |
| dc.okm.internationality | International publication | |
| dc.okm.type | A1 ScientificArticle | |
| dc.publisher | EDP SCIENCES S A | |
| dc.publisher.country | France | en_GB |
| dc.publisher.country | Ranska | fi_FI |
| dc.publisher.country-code | FR | |
| dc.relation.articlenumber | ARTN A69 | |
| dc.relation.doi | 10.1051/0004-6361/201423428 | |
| dc.relation.ispartofjournal | Astronomy and Astrophysics | |
| dc.relation.volume | 577 | |
| dc.source.identifier | https://www.utupub.fi/handle/10024/169788 | |
| dc.title | The physical state of selected cold clumps | |
| dc.year.issued | 2015 |
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