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[PDF] Top 20 The Companion Mass Function across the Stellar and Substellar Regime

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The Companion Mass Function across the Stellar and Substellar Regime

The Companion Mass Function across the Stellar and Substellar Regime

... of companion with masses between 10-40 M J upiter has been noticed at close separations, suggesting the possibility of a distinct formation mech- anism for objects above and below this ...planets ... Voir le document complet

148

Binary Formation Mechanisms: Constraints from the Companion Mass Ratio Distribution

Binary Formation Mechanisms: Constraints from the Companion Mass Ratio Distribution

... clusters and associations: general – stars: formation – stars: luminosity function, mass function – stars: pre-main sequence ...INTRODUCTION The study of binary stellar systems ... Voir le document complet

8

Stellar and substellar companions of nearby stars from Gaia DR2

Stellar and substellar companions of nearby stars from Gaia DR2

... Conclusion The combination of the Hipparcos and Gaia DR2 positions provides extremely accurate long-term PM vectors for a large number of ...stars. The improved parameters from the Gaia ... Voir le document complet

24

The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at $0.5 < z < 1.1$

The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at $0.5 < z < 1.1$

... ). The aim of this paper is to push these investigations to higher ...analyse the VIPERS Public Data Release 1 (PDR-1) ( Guzzo et ...straining the dependence of the 3PCF on stellar ... Voir le document complet

13

Characterization of low-mass companion HD 142527 B

Characterization of low-mass companion HD 142527 B

... M stellar companion evaded de- tection until recently causes us to question the prevalence of gapped disks where a binary or massive companion has not been detected ...at the origin of ... Voir le document complet

21

Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core mass function

Possible link between the power spectrum of interstellar filaments and the origin of the prestellar core mass function

... Although the thermal Jeans mass within marginally super- critical filaments may account for the peak of the prestellar CMF, pure thermal fragmentation of filaments at the thresh- old of ... Voir le document complet

11

AN AGE CONSTRAINT FOR THE VERY LOW MASS STELLAR/BROWN DWARF BINARY 2MASS J03202839-0446358AB

AN AGE CONSTRAINT FOR THE VERY LOW MASS STELLAR/BROWN DWARF BINARY 2MASS J03202839-0446358AB

... this mass/age degeneracy with- out resorting to atmospheric ...ric and/or spectroscopic orbit measurements, and com- ponent spectral types, effective temperatures and/or lu- minosities ... Voir le document complet

9

Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z ~ 1

Evidence for the inside-out growth of the stellar mass distribution in galaxy clusters since z ~ 1

... show the blue galaxy population of this sample, and also the blue galaxy population in the GCLASS clusters (vdB14, their ...in the relative radial distribution of blue galaxies compared ... Voir le document complet

16

Characterizing planet-hosting stars: how to get stellar mass, radius, and age

Characterizing planet-hosting stars: how to get stellar mass, radius, and age

... The targets of CHEOPS Main sequence nearby bright solar-like stars: F, G, and K-types Direct techniques: interferometry (R * ), eclipsing binaries (M * , R * ) Indirect techniques: GAIA parallaxes (R * ), ... Voir le document complet

15

Ice decay and the ice regime system

Ice decay and the ice regime system

... air and, depending upon the temperature, solid ...upon the prevailing conditions. The details of the ice microstructure influence significantly the mechanical and physical ... Voir le document complet

34

Constraining the efficiency of angular momentum transport   with asteroseismology of red giants: the effect of stellar mass

Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass

... 9). The low efficiency of the transport of angular momen- tum by meridional currents and the shear instability in radiative zones leads to a large increase in the core rotation rate ... Voir le document complet

12

Possible planet formation in the young, low-mass, multiple stellar system GG Tau A

Possible planet formation in the young, low-mass, multiple stellar system GG Tau A

... using the best data available (3 mm and ...derive the best fit 37 . The analysis is performed in the Fourier plane to avoid non linear effects due to the ...Fig.4 and ... Voir le document complet

32

The empirical mass distribution of hot B subdwarfs: implications for stellar evolution theory

The empirical mass distribution of hot B subdwarfs: implications for stellar evolution theory

... compact, and evolved objects that form the very hot end of the horizontal branch, the so-called Extreme Horizontal Branch ...Understanding the formation of sdB stars is one of ... Voir le document complet

8

Cosmological constraints from the virial mass function of nearby galaxy groups and clusters

Cosmological constraints from the virial mass function of nearby galaxy groups and clusters

... After removing foreground and background galaxies (interlopers) using a dynamical maximum-velocity criterion, I estimate the group and cluster masses using the full virial theo[r] ... Voir le document complet

82

The cold Leidenfrost regime

The cold Leidenfrost regime

... temperature and ap- proaching the boiling point oppose the formation of water nuclei in the texture, which contributes to lower ...imaging the bottom interface of the ... Voir le document complet

7

The distance and neutral environment of the massive stellar cluster Westerlund 1

The distance and neutral environment of the massive stellar cluster Westerlund 1

... motion and the possible occurence of a spiral ...predicts the location of the Tangent point gas and the velocity of the Sagittarius Arm outside the solar circle on ... Voir le document complet

2

Role of vapor mass transfer in flow coating of colloidal dispersions in the evaporative regime

Role of vapor mass transfer in flow coating of colloidal dispersions in the evaporative regime

... of the meniscus size. However the case of colloidal dispersions deserves further ...Indeed, the coating flow leads to a wet film of densely-packed colloids before the formation of the ... Voir le document complet

17

The distance and neutral environment of the massive stellar cluster Westerlund 1

The distance and neutral environment of the massive stellar cluster Westerlund 1

... in the Scutum-Crux I ...be the presence of non-circular ...to the line of sight towards Wd 1 assuming a distance of ...towards the Galactic cen- tre. At the location of Wd 1 the ... Voir le document complet

9

MEMORIZATION PERFORMANCE AS A FUNCTION OF ENCODING MODALITY ACROSS THE SHIFT WORKERS’ 24-HOUR DAY

MEMORIZATION PERFORMANCE AS A FUNCTION OF ENCODING MODALITY ACROSS THE SHIFT WORKERS’ 24-HOUR DAY

... grative and Comparative Physiology, 277, 1152-1153. RÉSUMÉ Les effets de la modalité de présentation (auditive vs visuelle) sur la mémorisation sont explorés chez des travailleurs postés à 3, 7, 11, 15, 19 et 23 ... Voir le document complet

21

The close-in companion of the fast rotating Be star Achernar

The close-in companion of the fast rotating Be star Achernar

... inside the wings of the PSF of ...to the good circular symme- try of the PSF produced by ...measure the photometry of A and B over the same aperture and within ... Voir le document complet

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