Change search
ReferencesLink to record
Permanent link

Direct link
M-dwarf binaries as tracers of star and brown dwarf formation
Stockholm University, Faculty of Science, Department of Astronomy.
Show others and affiliations
Number of Authors: 5
2015 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 452, no 1, 1014-1025 p.Article in journal (Refereed) Published
Abstract [en]

The separation distribution for M-dwarf binaries in the AstraLux survey is narrower and peaking at smaller separations than the distribution for solar-type binaries. This is often interpreted to mean that M-dwarfs constitute a continuous transition from brown dwarfs (BDs) to stars. Here, a prediction for the M-dwarf separation distribution is presented, using a dynamical population synthesis (DPS) model in which 'star-like' binaries with late-type primaries (less than or similar to 1.5 M-circle dot) follow universal initial distribution functions and are dynamically processed in their birth embedded clusters. A separate 'BD-like' population has both its own distribution functions for binaries and initial mass function (IMF), which overlaps in mass with the IMF for stars. Combining these two formation modes results in a peak on top of a wider separation distribution for late M-dwarfs consistent with the late AstraLux sample. The DPS separation distribution for early M-dwarfs shows no such peak and is in agreement with the M-dwarfs in Multiples (MinMS) data. We note that the latter survey is potentially in tension with the early AstraLux data. Concluding, the AstraLux and MinMS data are unable to unambiguously distinguish whether or not BDs are a continuous extension of the stellar IMF. Future observational efforts are needed to fully answer this interesting question. The DPS model predicts that binaries outside the sensitivity range of the AstraLux survey remain to be detected. For application to future data, we present a means to observationally measure the overlap of the putative BD-like branch and the stellar branch. We discuss the meaning of universal star formation and distribution functions.

Place, publisher, year, edition, pages
2015. Vol. 452, no 1, 1014-1025 p.
Keyword [en]
binaries: general, stars: formation, stars: kinematics and dynamics, stars: late-type, stars: low-mass
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-121674DOI: 10.1093/mnras/stv1361ISI: 000360851100078OAI: oai:DiVA.org:su-121674DiVA: diva2:889949
Available from: 2015-12-29 Created: 2015-10-13 Last updated: 2015-12-29Bibliographically approved

Open Access in DiVA

No full text

Other links

Publisher's full text

Search in DiVA

By author/editor
Janson, Markus
By organisation
Department of Astronomy
In the same journal
Monthly notices of the Royal Astronomical Society
Physical Sciences

Search outside of DiVA

GoogleGoogle Scholar
The number of downloads is the sum of all downloads of full texts. It may include eg previous versions that are now no longer available

Altmetric score

Total: 6 hits
ReferencesLink to record
Permanent link

Direct link