Matches in SemOpenAlex for { <https://semopenalex.org/work/W1535765562> ?p ?o ?g. }
Showing items 1 to 46 of
46
with 100 items per page.
- W1535765562 endingPage "128" @default.
- W1535765562 startingPage "112" @default.
- W1535765562 abstract "Virtually all stars are born with neighbors. Most stellar systems are multiple, and many if not most stars are born in groups, with a subset in clusters of substantial numbers of stars. An understanding of multiplicity is therefore an important part of theories of star formation. The complex structure within molecular clouds, and in particular the asymmetries present in protostellar cores, may be essential to understanding the process of forming binaries. Whether the disks formed during protostellar collapse are capable of spawning multiple stellar companions rather than simply accreting onto the central object is an open question, perhaps requiring strong departures from axisymmetry in the infalling material. Observationally, we detect multiple protostellar systems which appear to lie within disks or toroids in Class I sources, indicating that stellar fragmentation occurs before infall to the disk is complete. The early evolution of binary and multiple stellar systems is likely to be complex. The growth in mass of fragments formed early on will depend upon complicated accretion processes in disks and infalling envelopes. If more than two fragments are formed, the system can become dynamically unstable, resulting in dispersal or ejection of some members. Whether many or even any stars are initially formed as single objects, or instead were ejected from multiple systems, is currently unclear. Probably most young stars are born in clusters or groups. Currently most stars in the solar neigborhood are born in modest-sized groups of order 10–100 members in regions of order a pc in size." @default.
- W1535765562 created "2016-06-24" @default.
- W1535765562 creator A5053918712 @default.
- W1535765562 date "2008-11-20" @default.
- W1535765562 modified "2023-09-23" @default.
- W1535765562 title "Binaries, clusters, and the IMF" @default.
- W1535765562 doi "https://doi.org/10.1017/cbo9780511552090.008" @default.
- W1535765562 hasPublicationYear "2008" @default.
- W1535765562 type Work @default.
- W1535765562 sameAs 1535765562 @default.
- W1535765562 citedByCount "0" @default.
- W1535765562 crossrefType "book-chapter" @default.
- W1535765562 hasAuthorship W1535765562A5053918712 @default.
- W1535765562 hasConcept C121332964 @default.
- W1535765562 hasConcept C44870925 @default.
- W1535765562 hasConceptScore W1535765562C121332964 @default.
- W1535765562 hasConceptScore W1535765562C44870925 @default.
- W1535765562 hasLocation W15357655621 @default.
- W1535765562 hasOpenAccess W1535765562 @default.
- W1535765562 hasPrimaryLocation W15357655621 @default.
- W1535765562 hasRelatedWork W1495579573 @default.
- W1535765562 hasRelatedWork W1496971617 @default.
- W1535765562 hasRelatedWork W1584002683 @default.
- W1535765562 hasRelatedWork W1600379717 @default.
- W1535765562 hasRelatedWork W1620491751 @default.
- W1535765562 hasRelatedWork W164437351 @default.
- W1535765562 hasRelatedWork W1972465580 @default.
- W1535765562 hasRelatedWork W1983924390 @default.
- W1535765562 hasRelatedWork W2007040111 @default.
- W1535765562 hasRelatedWork W2009503507 @default.
- W1535765562 hasRelatedWork W2034534553 @default.
- W1535765562 hasRelatedWork W2762773434 @default.
- W1535765562 hasRelatedWork W2949887751 @default.
- W1535765562 hasRelatedWork W2960650723 @default.
- W1535765562 hasRelatedWork W3036149647 @default.
- W1535765562 hasRelatedWork W3099747735 @default.
- W1535765562 hasRelatedWork W3103105867 @default.
- W1535765562 hasRelatedWork W3103660106 @default.
- W1535765562 hasRelatedWork W3104907640 @default.
- W1535765562 hasRelatedWork W3020857061 @default.
- W1535765562 isParatext "false" @default.
- W1535765562 isRetracted "false" @default.
- W1535765562 magId "1535765562" @default.
- W1535765562 workType "book-chapter" @default.