Search Publications

Microphysics of KCl and ZnS Clouds on GJ 1214 b
DOI: 10.3847/1538-4357/aad461 Bibcode: 2018ApJ...863..165G

Benneke, Björn; Gao, Peter

Clouds in the atmospheres of exoplanets confound characterization efforts by reducing, eliminating, and distorting the spectral signatures of molecular abundances. As such, interpretations of exoplanet spectra strongly depend on the choice of cloud model, many of which are highly simplified and lack predictive power. In this work, we use a cloud m…

2018 The Astrophysical Journal
eHST 76
Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z ∼ 0.8 Quiescent Galaxies
DOI: 10.3847/1538-4357/aabc55 Bibcode: 2018ApJ...858...60B

Bell, Eric F.; Maseda, Michael V.; Franx, Marijn +18 more

We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at z = 0.6-1 from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic survey. Rotation is typically probed across 10-20 kpc, or to an average of 2.7Re. Combined with central stellar velocity dispersions (σ0) this provi…

2018 The Astrophysical Journal
eHST 76
Resolving Quiescent Galaxies at z ≳ 2. II. Direct Measures of Rotational Support
DOI: 10.3847/1538-4357/aacd4f Bibcode: 2018ApJ...862..126N

Ellis, Richard S.; Belli, Sirio; Newman, Andrew B. +1 more

Stellar kinematics provide insights into the masses and formation histories of galaxies. At high redshifts, spatially resolving the stellar kinematics of quiescent galaxies is challenging due to their compact sizes. Using deep near-infrared spectroscopy, we have measured the resolved stellar kinematics of four quiescent galaxies at z = 1.95-2.64, …

2018 The Astrophysical Journal
eHST 76
Far-ultraviolet Activity Levels of F, G, K, and M Dwarf Exoplanet Host Stars
DOI: 10.3847/1538-4365/aae1a3 Bibcode: 2018ApJS..239...16F

Loyd, R. O. Parke; Redfield, Seth; France, Kevin +4 more

We present a survey of far-ultraviolet (FUV; 1150-1450 Å) emission line spectra from 71 planet-hosting and 33 non-planet-hosting F, G, K, and M dwarfs with the goals of characterizing their range of FUV activity levels, calibrating the FUV activity level to the 90-360 Å extreme-ultraviolet (EUV) stellar flux, and investigating the potential for FU…

2018 The Astrophysical Journal Supplement Series
eHST 76
A Gap in the Lower Main Sequence Revealed by Gaia Data Release 2
DOI: 10.3847/2041-8213/aacdf6 Bibcode: 2018ApJ...861L..11J

Gies, Douglas R.; Henry, Todd J.; Jao, Wei-Chun +1 more

We present the discovery of a gap near M G ≈ 10 in the main sequence on the Hertzsprung-Russell Diagram (HRD) based on measurements presented in Gaia Data Release 2 (DR2). Using an observational form of the HRD with M G representing luminosity and G BP - G RP representing temperature, the gap present…

2018 The Astrophysical Journal
Gaia 75
Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K-primaries - I: High-resolution spectroscopy with HERMES: stellar parameters, abundances, and kinematics
DOI: 10.1093/mnras/sty1295 Bibcode: 2018MNRAS.479.1332M

Alonso-Floriano, F. J.; Caballero, J. A.; Montes, D. +7 more

We investigated almost 500 stars distributed among 193 binary or multiple systems made of late-F, G-, or early-K-primaries and late-K- or M-dwarf companion candidates. For all of them, we compiled or measured coordinates, J-band magnitudes, spectral types, distances, and proper motions. With these data, we established a sample of 192 physically bo…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 75
Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing
DOI: 10.1051/0004-6361/201731361 Bibcode: 2018A&A...613A..12M

Puls, J.; Langer, N.; Markova, N.

Context. Massive stars play a key role in the evolution of galaxies and our Universe.
Aims: Our goal is to compare observed and predicted properties of single Galactic O stars to identify and constrain uncertain physical parameters and processes in stellar evolution and atmosphere models.
Methods: We used a sample of 53 objects of all lu…

2018 Astronomy and Astrophysics
Gaia 75
Old-Aged Primary Distance Indicators
DOI: 10.1007/s11214-018-0542-1 Bibcode: 2018SSRv..214..113B

Salaris, Maurizio; Matsunaga, Noriyuki; Beaton, Rachael L. +8 more

Old-aged stellar distance indicators are present in all Galactic structures (halo, bulge, disk) and in galaxies of all Hubble types and, thus, are immensely powerful tools for understanding our Universe. Here we present a comprehensive review for three primary standard candles from Population II: (i) RR Lyrae type variables (RRL), (ii) type II Cep…

2018 Space Science Reviews
Gaia 75
Fast Estimation of Orbital Parameters in Milky Way-like Potentials
DOI: 10.1088/1538-3873/aadcdd Bibcode: 2018PASP..130k4501M

Bovy, Jo; Mackereth, J. Ted

Orbital parameters, such as eccentricity and maximum vertical excursion, of stars in the Milky Way are an important tool for understanding its dynamics and evolution, but calculation of such parameters usually relies on computationally expensive numerical orbit integration. We present and test a fast method for estimating these parameters using an…

2018 Publications of the Astronomical Society of the Pacific
Gaia 75
Revised Gaia Data Release 2 passbands
DOI: 10.1051/0004-6361/201833462 Bibcode: 2018A&A...617A.138W

Weiler, Michael

Context. The European Space Agency mission Gaia has published, with its second data release (DR2), a catalogue of photometric measurements for more than 1.3 billion astronomical objects in three passbands. The precision of the measurements in these passbands, denoted G, GBP, and GRP, reach down to the milli-magnitude level. T…

2018 Astronomy and Astrophysics
Gaia eHST 75