Search Publications

Constraints on Upper Cutoffs in the Mass Functions of Young Star Clusters
DOI: 10.3847/1538-4357/aaf6ea Bibcode: 2019ApJ...872...93M

Fall, S. Michael; Chandar, Rupali; Mok, Angus

We test claims that the power-law mass functions of young star clusters (ages ≲ few × 108 yr) have physical upper cutoffs at {M}* ∼ {10}5 {M}. Specifically, we perform maximum likelihood fits of the Schechter function, \psi (M)={dN}/{dM}\propto {M}β \exp (-M/{M}* ), to the observe…

2019 The Astrophysical Journal
eHST 37
M I C R O S C O P E limits on the strength of a new force with comparisons to gravity and electromagnetism
DOI: 10.1103/PhysRevD.99.055043 Bibcode: 2019PhRvD..99e5043F

Fayet, Pierre

Extremely weak new forces could lead to apparent violations of the equivalence principle. The MICROSCOPE experiment implies that the relative strength of a new long-range force, compared with gravity, is constrained to |α¯ g|<3.2 ×10-11 , 2.3 ×10-13 , 2.2 ×10-13 , 6.7 ×10-13 , and 1.5 ×10

2019 Physical Review D
MICROSCOPE 37
Abundances of disk and bulge giants from high-resolution optical spectra. IV. Zr, La, Ce, Eu
DOI: 10.1051/0004-6361/201936343 Bibcode: 2019A&A...631A.113F

Ryde, N.; Jönsson, H.; Matteucci, F. +1 more

Context. Observations of the Galactic bulge suggest that the disk formed through secular evolution rather than gas dissipation and/or mergers, as previously believed. This would imply very similar chemistry in the disk and bulge. Some elements, such as the α-elements, are well studied in the bulge, but others like the neutron-capture elements are …

2019 Astronomy and Astrophysics
Gaia 37
Cloud Atlas: Hubble Space Telescope Near-infrared Spectral Library of Brown Dwarfs, Planetary-mass Companions, and Hot Jupiters
DOI: 10.3847/1538-3881/aaf88f Bibcode: 2019AJ....157..101M

Schneider, Glenn; Apai, Dániel; Burgasser, Adam J. +12 more

Bayesian atmospheric retrieval tools can place constraints on the properties of brown dwarfs' and hot Jupiters' atmospheres. To fully exploit these methods, high signal-to-noise spectral libraries with well-understood uncertainties are essential. We present a high signal-to-noise spectral library (1.10-1.69 µm) of the thermal emission of 76 …

2019 The Astronomical Journal
Gaia eHST 37
Modelling depletion by re-accretion of gas from a dusty disc in post-AGB stars
DOI: 10.1051/0004-6361/201935853 Bibcode: 2019A&A...629A..49O

Van Winckel, Hans; Nelemans, Gijs; Pols, Onno +1 more

Many disc-type post-asymptotic giant branch (post-AGB) stars are chemically peculiar, showing underabundances of refractory elements in their photospheres that correlate with condensation temperature. The aim of this paper is to investigate how accretion from a circumbinary disc can cause this phenomenon of depletion and how this impacts the evolu…

2019 Astronomy and Astrophysics
Gaia 37
Properties of Radial Velocities Measurement Based on LAMOST-II Medium-resolution Spectroscopic Observations
DOI: 10.3847/1538-4365/ab3cc0 Bibcode: 2019ApJS..244...27W

Wu, H.; Chen, L.; Wang, R. +28 more

The radial velocity (RV) is a basic physical quantity that can be determined through the Doppler shift of the spectrum of a star. The precision of the RV measurement depends on the resolution of the spectrum we used and the accuracy of wavelength calibration. In this work, radial velocities of the Large Sky Area Multi-Object Fibre Spectroscopic Te…

2019 The Astrophysical Journal Supplement Series
Gaia 37
Quiescent Discrete Auroral Arcs: A Review of Magnetospheric Generator Mechanisms
DOI: 10.1007/s11214-019-0619-5 Bibcode: 2019SSRv..216....1B

Echim, Marius M.; Borovsky, Joseph E.; Otto, Antonius +7 more

One of the longstanding questions of space science is: How does the Earth's magnetosphere generate auroral arcs? A related question is: What form of energy is extracted from the magnetosphere to drive auroral arcs? Not knowing the answers to these questions hinders our ability to determine the impact of auroral arcs on the magnetospheric system. M…

2019 Space Science Reviews
Cluster 37
Homogeneously derived transit timings for 17 exoplanets and reassessed TTV trends for WASP-12 and WASP-4
DOI: 10.1093/mnras/stz2620 Bibcode: 2019MNRAS.490.1294B

Molina, D.; Bretton, M.; Jones, H. R. A. +34 more

We homogeneously analyse ∼3.2 × 105 photometric measurements for ∼1100 transit light curves belonging to 17 exoplanet hosts. The photometric data cover 16 years (2004-2019) and include amateur and professional observations. Old archival light curves were reprocessed using up-to-date exoplanetary parameters and empirically debiased limb-…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 37
Multifractal and Chaotic Properties of Solar Wind at MHD and Kinetic Domains: An Empirical Mode Decomposition Approach
DOI: 10.3390/e21030320 Bibcode: 2019Entrp..21..320A

Marcucci, Maria Federica; Consolini, Giuseppe; Alberti, Tommaso +3 more

Turbulence, intermittency, and self-organized structures in space plasmas can be investigated by using a multifractal formalism mostly based on the canonical structure function analysis with fixed constraints about stationarity, linearity, and scales. Here, the Empirical Mode Decomposition (EMD) method is firstly used to investigate timescale fluc…

2019 Entropy
Cluster 37
Constraining the evolution of stellar rotation using solar twins
DOI: 10.1093/mnrasl/slz034 Bibcode: 2019MNRAS.485L..68L

Bedell, Megan; Meléndez, Jorge; Bean, Jacob L. +7 more

The stellar rotation versus age relation is commonly considered a useful tool to derive reliable ages for Sun-like stars. However, in the light of Kepler data, the presence of apparently old and fast rotators that do not obey the usual gyrochronology relations led to the hypothesis of weakened magnetic breaking in some stars. In this letter, we co…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 37