onr:"swepub:oai:research.chalmers.se:b9fa986c-bb91-46b3-8480-9e2ab6d9ddf8"
Sökning: onr:"swepub:oai:research.chalmers.se:b9fa986c-bb91-46b3-8480-9e2ab6d9ddf8" > (2016) > AN M DWARF COMPANIO...
- 1 av 1
- Föregående post
- Nästa post
- Till träfflistan
| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 03950naa a2200493 4500 | |
| 001 | oai:research.chalmers.se:b9fa986c-bb91-46b3-8480-9e2ab6d9ddf8 | |
| 003 | SwePub | |
| 008 | 171008s2016 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://doi.org/10.3847/0004-6256/151/3/842 DOI |
| 024 | 7 | a https://research.chalmers.se/publication/2338852 URI |
| 040 | a (SwePub)cth | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a art2 swepub-publicationtype |
| 072 | 7 | a ref2 swepub-contenttype |
| 100 | 1 | a Eigmüller, Philippu Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR),Thüringer Landessternwarte Tautenburg4 aut |
| 245 | 1 0 | a AN M DWARF COMPANION TO AN F-TYPE STAR IN A YOUNG MAIN-SEQUENCE BINARY |
| 264 | c 2016-02-26 | |
| 264 | 1 | b American Astronomical Society,c 2016 |
| 338 | a electronic2 rdacarrier | |
| 520 | a Only a few well characterized very low-mass M dwarfs are known today. Our understanding of M dwarfs is vital as these are the most common stars in our solar neighborhood. We aim to characterize the properties of a rare F+dM stellar system for a better understanding of the low-mass end of the Hertzsprung-Russel diagram. We used photometric light curves and radial velocity follow-up measurements to study the binary. Spectroscopic analysis was used in combination with isochrone fitting to characterize the primary star. The primary star is an early F-type main-sequence star with a mass of (1.493 +/- 0.073) M-circle dot and a radius of (1.474 +/- 0.040) R-circle dot. The companion is an M dwarf with a mass of (0.188 +/- 0.014) M-circle dot and a radius of (0.234 +/- 0.009) R-circle dot. The orbital period is (1.35121 +/- 0.00001) days. The secondary star is among the lowest-mass M dwarfs known to date. The binary has not reached a 1: 1 spin-orbit synchronization. This indicates a young main-sequence binary with an age below similar to 250 Myr. The mass-radius relation of both components are in agreement with this finding. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a stars: evolution | |
| 653 | a binaries: eclipsing | |
| 653 | a stars: low-mass | |
| 653 | a binaries: close | |
| 700 | 1 | a Eisloffel, J.u Thüringer Landessternwarte Tautenburg4 aut |
| 700 | 1 | a Csizmadia, S.u Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)4 aut |
| 700 | 1 | a Lehmann, H.u Thüringer Landessternwarte Tautenburg4 aut |
| 700 | 1 | a Erikson, A.u Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)4 aut |
| 700 | 1 | a Fridlund, Malcolm,d 1952u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)malfri |
| 700 | 1 | a Hartmann, M.u Thüringer Landessternwarte Tautenburg4 aut |
| 700 | 1 | a Hatzes, A.u Thüringer Landessternwarte Tautenburg4 aut |
| 700 | 1 | a Pasternacki, T.u Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)4 aut |
| 700 | 1 | a Rauer, H.u Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR),Technische Universität Berlin4 aut |
| 700 | 1 | a Tkachenko, A.u Katholieke Universiteit Leuven4 aut |
| 700 | 1 | a Voss, H.u Universitat de Barcelona,University of Barcelona4 aut |
| 710 | 2 | a Deutsches Zentrums für Luft- und Raumfahrt (DLR)b Thüringer Landessternwarte Tautenburg4 org |
| 773 | 0 | t Astronomical Journald : American Astronomical Societyg 151:3q 151:3x 1538-3881x 0004-6256 |
| 856 | 4 | u http://publications.lib.chalmers.se/records/fulltext/233885/local_233885.pdfx primaryx freey FULLTEXT |
| 856 | 4 | u https://lirias.kuleuven.be/bitstream/123456789/575221/1/1602.01575.pdf |
| 856 | 4 8 | u https://doi.org/10.3847/0004-6256/151/3/84 |
| 856 | 4 8 | u https://research.chalmers.se/publication/233885 |
- 1 av 1
- Föregående post
- Nästa post
- Till träfflistan
Hitta mer i SwePub
- Av författaren/redakt...
- Eigmüller, Phili ...
- Eisloffel, J.
- Csizmadia, S.
- Lehmann, H.
- Erikson, A.
- Fridlund, Malcol ...
- visa fler...
- Hartmann, M.
- Hatzes, A.
- Pasternacki, T.
- Rauer, H.
- Tkachenko, A.
- Voss, H.
- visa färre...
- Om ämnet
-
- NATURVETENSKAP
- NATURVETENSKAP
- och Fysik
- och Astronomi astrof ...
- Artiklar i publikationen
- Astronomical Jou ...
- Av lärosätet
- Chalmers tekniska högskola
Sök utanför SwePub
- Sök vidare i:
- Google Book Search
- Google Scholar
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
- Copyright © LIBRIS - Nationella bibliotekssystem
- LIBRIS.kb.se
