Search Publications

Statistics of Wide Pre-main-sequence Binaries in the Orion OB1 Association
DOI: 10.3847/1538-3881/abc2d6 Bibcode: 2020AJ....160..268T

Tokovinin, Andrei; Petr-Gotzens, Monika G.; Briceño, Cesar

Statistics of low-mass pre-main-sequence binaries in the Orion OB1 association with separations ranging from 0"6 to 20″ (220 to 7400 au at 370 pc) are studied using images from the VISTA Orion mini survey and astrometry from Gaia. The input sample based on the CVSO catalog contains 1137 stars of K and M spectral types (masses between 0.3 and 0.9 $…

2020 The Astronomical Journal
Gaia 15
Multiple Explanations for the Single Transit of KIC 5951458 Based on Radial Velocity Measurements Extracted with a Novel Matched-template Technique
DOI: 10.3847/1538-3881/abad27 Bibcode: 2020AJ....160..149D

Kane, Stephen R.; Howard, Andrew W.; Dalba, Paul A. +2 more

Planetary systems that show single-transit events are a critical pathway to increasing the yield of long-period exoplanets from transit surveys. From the primary Kepler mission, KIC 5951458 b (Kepler-456b) was thought to be a single-transit giant planet with an orbital period of 1310 days. However, radial velocity (RV) observations of KIC 5951458 …

2020 The Astronomical Journal
Gaia 15
On the Metamorphosis of the Bailey Diagram for RR Lyrae Stars
DOI: 10.3847/2041-8213/ab9538 Bibcode: 2020ApJ...896L..15B

Kovtyukh, V.; Lemasle, B.; Walker, A. R. +37 more

We collected over 6000 high-resolution spectra of four dozen field RR Lyrae (RRL) variables pulsating either in the fundamental (39 RRab) or in the first overtone (9 RRc) mode. We measured radial velocities (RVs) of four strong metallic and four Balmer lines along the entire pulsational cycle and derived RV amplitudes with accuracies better than 1…

2020 The Astrophysical Journal
Gaia 15
Revisiting the Magnetic Field of the L183 Starless Core
DOI: 10.3847/1538-4357/abad37 Bibcode: 2020ApJ...900..181K

Karoly, Janik; Bastien, Pierre; Coudé, Simon +4 more

We present observations of linear polarization from dust thermal emission at 850 µm toward the starless cloud L183. These data were obtained at the James Clerk Maxwell Telescope (JCMT) using the SCUBA-2 camera in conjunction with its polarimeter POL-2. Polarized dust emission traces the plane-of-sky magnetic field structure in the cloud, thu…

2020 The Astrophysical Journal
Herschel 15
The Inner Disk of RY Tau: Evidence of Stellar Occultation by the Disk Atmosphere at the Sublimation Rim from K-band Continuum Interferometry
DOI: 10.3847/1538-4357/ab93c1 Bibcode: 2020ApJ...897...31D

Monnier, John D.; Kraus, Stefan; Baron, Fabien +13 more

We present models of the inner region of the circumstellar disk of RY Tau that aim to explain our near-infrared (K-band: 2.1 µm) interferometric observations, while remaining consistent with the optical to near-infrared portions of the spectral energy distribution. Our submilliarcsecond-resolution CHARA Array observations are supplemented wi…

2020 The Astrophysical Journal
Gaia 15
Non-stoichiometric amorphous magnesium-iron silicates in circumstellar dust shells. Dust growth in outflows from supergiants
DOI: 10.1051/0004-6361/202038090 Bibcode: 2020A&A...644A.139G

Tamanai, Akemi; Pucci, Annemarie; Dohmen, Ralf +1 more


Aims: We study the growth of dust in oxygen-rich stellar outflows in order to find out to which extent dust growth models can quantitatively reconcile with the quantities and nature of dust as derived from observations of the infrared emission from circumstellar dust shells.
Methods: We use a set of nine well-observed massive supergiants…

2020 Astronomy and Astrophysics
ISO 15
Mapping the Galactic Disk with the LAMOST and Gaia Red Clump Sample. IV. The Kinematic Signature of the Galactic Warp
DOI: 10.3847/1538-4357/aba61e Bibcode: 2020ApJ...901...56L

Wang, H. -F.; Huang, Y.; Chen, B. -Q. +5 more

Using a sample of nearly 140,000 red clump stars selected from the LAMOST and Gaia Galactic surveys, we have mapped mean vertical velocity $\overline{{V}_{z}}$ in the X-Y plane for a large volume of the Galactic disk (6 < R < 16 kpc; -20 < φ < 50°; $| Z| \lt 1$ kpc). A clear signature where $\overline{{V}_{z}}$ increases with R is dete…

2020 The Astrophysical Journal
Gaia 15
Low-cost precursor of an interstellar mission
DOI: 10.1051/0004-6361/202038687 Bibcode: 2020A&A...641A..45H

Heller, René; Hippke, Michael; Kervella, Pierre +1 more

The solar photon pressure provides a viable source of thrust for spacecraft in the solar system. Theoretically it could also enable interstellar missions, but an extremely small mass per cross section area is required to overcome the solar gravity. We identify aerographite, a synthetic carbon-based foam with a density of 0.18 kg m-3 (15…

2020 Astronomy and Astrophysics
Gaia 15
Improved Infrared Photometry and a Preliminary Parallax Measurement for the Extremely Cold Brown Dwarf CWISEP J144606.62-231717.8
DOI: 10.3847/2041-8213/ab6201 Bibcode: 2020ApJ...888L..19M

Meisner, Aaron M.; Cushing, Michael C.; Kirkpatrick, J. Davy +6 more

We present follow-up Spitzer observations at 3.6 µm (ch1) and 4.5 µm (ch2) of CWISEP J144606.62-231717.8, one of the coldest known brown dwarfs in the solar neighborhood. This object was found by mining the Wide-field Infrared Survey Explorer (WISE) and NEOWISE data via the CatWISE Preliminary Catalog by Meisner et al., where an initia…

2020 The Astrophysical Journal
Gaia 15
First detection of NHD and ND2 in the interstellar medium. Amidogen deuteration in IRAS 16293-2422
DOI: 10.1051/0004-6361/202038490 Bibcode: 2020A&A...641A.153M

Caselli, P.; Sipilä, O.; Bizzocchi, L. +7 more

Context. Deuterium fractionation processes in the interstellar medium (ISM) have been shown to be highly efficient in the family of nitrogen hydrides. To date, observations have been limited to ammonia (NH2D, NHD2, ND3) and imidogen radical (ND) isotopologues.
Aims: We want to explore the high-frequency window…

2020 Astronomy and Astrophysics
Herschel 15