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Astronomy and Astrophysics, ISSN 0004-6361, 10/2010, Volume 520, Issue 9, p. A54
Context. While M dwarfs are the most abundant stars in the Milky Way, there is still large uncertainty about their basic physical properties (mass, luminosity,... 
binaries: visual | techniques: high angular resolution | brown dwarfs | stars: low-mass | GIANT PLANETS | ADAPTIVE OPTICS | STAR-FORMATION | SOLAR NEIGHBORHOOD | ASTRONOMY & ASTROPHYSICS | NEARBY | SKY SURVEY | COMPANIONS | MOVING GROUP | LOW-MASS BINARIES | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2018, Volume 620, p. A33
Low-mass stars exhibit substantial pre-main sequence evolution during the first ∼100 Myr of their lives. Thus, young M-type stars are prime targets for... 
Monitoring instruments | Binary stars | Luminosity | Bolometers | Evolution | Stellar evolution | Pre-main sequence stars | M stars | Empirical analysis | Stellar age | Low mass stars | Physics | Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 05/2018, Volume 613, p. L6
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2018, Volume 618, p. A23
A&A 618, A23 (2018) Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less... 
Techniques: high angular resolution | Stars: pre-main sequence | Binaries: visual | Stars: individual: GJ 2060 | Stars: low-mass | Stars: individual: TWA 22 | Astrometry
Journal Article
Journal of Applied Probability, ISSN 0021-9002, 12/2015, Volume 52, Issue 4, pp. 1146 - 1155
It is well known that the central limit theorem holds for partial sums of a stationary sequence (Xi) of m-dependent random variables with finite variance;... 
60C05 | 60G10 | m-dependent | stationary sequence | block factor | random tree | 60F05
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 3, pp. 2576 - 2585
Journal Article
Journal of Applied Probability, ISSN 0021-9002, 12/2015, Volume 52, Issue 4, pp. 1146 - 1155
It is well known that the central limit theorem holds for partial sums of a stationary sequence (Xi) of m-dependent random variables with finite variance;... 
Block factor | Stationary sequence | M-dependent | Random tree | STATISTICS & PROBABILITY | m-dependent | random tree | stationary sequence | block factor | Naturvetenskap | Mathematics | Natural Sciences | Matematik
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 626
Wide low-mass substellar companions are known to be very rare among low-mass stars, but appear to become increasingly common with increasing stellar mass.... 
PLANETS | POPULATION | BROWN DWARF DESERT | MEMBERS | LOW-MASS STARS | ROTATIONAL VELOCITIES | stars: early-type | 1ST | brown dwarfs | NAOS | SPECTROSCOPY | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | planets and satellites: detection | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Journal of Applied Probability, ISSN 0021-9002, 12/2015, Volume 52, Issue 4, p. 1146
  It is well known that the central limit theorem holds for partial sums of a stationary sequence (Xi) of m-dependent random variables with finite variance;... 
Studies | Theorems | Random variables | Stochastic models | Variance analysis
Journal Article
Journal of Applied Probability, ISSN 0021-9002, 12/2015, Volume 52, Issue 4, pp. 1146 - 1146
It is well known that the central limit theorem holds for partial sums of a stationary sequence (Xi) of m-dependent random variables with finite variance;... 
Mathematical analysis | Symbols | Blocking | Random variables | Criteria | Variance | Counting | Sums
Journal Article
Astronomy and Astrophysics - A&A, ISSN 0004-6361, 2018, Volume 618, p. A23
Context. Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less reliable at... 
Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article