Search Publications

Compton-thick AGNs in the NuSTAR Era. III. A Systematic Study of the Torus Covering Factor
DOI: 10.3847/1538-4357/aafbeb Bibcode: 2019ApJ...872....8M

Cusumano, G.; Vignali, C.; Comastri, A. +9 more

We present the analysis of a sample of 35 candidate Compton-thick active galactic nuclei (AGNs) selected in the nearby universe (average redshift < z> ∼ 0.03) with the Swift-BAT 100-month survey. All sources have available NuSTAR data, thus allowing us to constrain with unprecedented quality important spectral parameters such as the obscurin…

2019 The Astrophysical Journal
XMM-Newton 40
Spectral and orbital characterisation of the directly imaged giant planet HIP 65426 b
DOI: 10.1051/0004-6361/201834112 Bibcode: 2019A&A...622A..80C

Queloz, D.; Quanz, S. P.; Avenhaus, H. +38 more

HIP 65426 b is a recently discovered exoplanet imaged during the course of the SPHERE-SHINE survey. Here we present new L' and M' observations of the planet from the NACO instrument at the VLT from the NACO-ISPY survey, as well as a new Y -H spectrum and K-band photometry from SPHERE-SHINE. Using these data, we confirm the nature of the companion …

2019 Astronomy and Astrophysics
Gaia Hipparcos 40
OCCASO - III. Iron peak and α elements of 18 open clusters. Comparison with chemical evolution models and field stars
DOI: 10.1093/mnras/stz2595 Bibcode: 2019MNRAS.490.1821C

Jordi, C.; Casamiquela, L.; Anders, F. +10 more

The study of open-cluster chemical abundances provides insights on stellar nucleosynthesis processes and on Galactic chemo-dynamical evolution. In this paper we present an extended abundance analysis of 10 species (Fe, Ni, Cr, V, Sc, Si, Ca, Ti, Mg, O) for red giant stars in 18 OCCASO clusters. This represents a homogeneous sample regarding the in…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 40
Upper limits on CH3OH in the HD 163296 protoplanetary disk. Evidence for a low gas-phase CH3OH-to-H2CO ratio
DOI: 10.1051/0004-6361/201834353 Bibcode: 2019A&A...623A.124C

Carpenter, J. M.; Walsh, C.; Hogerheijde, M. R. +6 more

Context. Methanol (CH3OH) is at the root of organic ice chemistry in protoplanetary disks. Its connection to prebiotic chemistry and its role in the chemical environment of the disk midplane make it an important target for disk chemistry studies. However, its weak emission has made detections difficult. To date, gas-phase CH3

2019 Astronomy and Astrophysics
Gaia 40
Combined Effects of Rotation and Age Spreads on Extended Main-Sequence Turn Offs
DOI: 10.3847/1538-4357/ab5717 Bibcode: 2019ApJ...887..199G

Dolphin, Andrew E.; Williams, Benjamin F.; Johnson, L. Clifton +10 more

The extended main-sequence turn offs (eMSTOs) of several young to intermediate age clusters are examined in the Magellanic Clouds and the Milky Way. We explore the effects of extended star formation (eSF) and a range of stellar rotation rates on the behavior of the color-magnitude diagram, paying particular attention to the MSTO. We create synthet…

2019 The Astrophysical Journal
Gaia eHST 40
The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
DOI: 10.3847/1538-4357/ab4263 Bibcode: 2019ApJ...885..141B

Madore, Barry F.; Freedman, Wendy L.; Beaton, Rachael L. +9 more

The Carnegie-Chicago Hubble Program (CCHP) is building a direct path to the Hubble constant (H 0) using Population II stars as the calibrator of the Type Ia supernova (SN Ia)-based distance scale. This path to calibrate the SNe Ia is independent of the systematics in the traditional Cepheid-based technique. In this paper, we present the…

2019 The Astrophysical Journal
eHST 40
HD 2685 b: a hot Jupiter orbiting an early F-type star detected by TESS
DOI: 10.1051/0004-6361/201834640 Bibcode: 2019A&A...625A..16J

Henning, Thomas; Vanderburg, Andrew; Latham, David W. +50 more

We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 ± 76 K) star HD 2685, whose transit signal was detected in Sector 1 data of NASA's TESS mission. We confirmed the planetary nature of the transit signal using Doppler velocimetric measurements with CHIRON, CORALIE, and FEROS, as well as usi…

2019 Astronomy and Astrophysics
Gaia 40
Hi-C 2.1 Observations of Jetlet-like Events at Edges of Solar Magnetic Network Lanes
DOI: 10.3847/2041-8213/ab594a Bibcode: 2019ApJ...887L...8P

Tiwari, Sanjiv K.; Winebarger, Amy R.; Warren, Harry P. +15 more

We present high-resolution, high-cadence observations of six, fine-scale, on-disk jet-like events observed by the High-resolution Coronal Imager 2.1 (Hi-C 2.1) during its sounding-rocket flight. We combine the Hi-C 2.1 images with images from the Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA) and the Interface Region Imaging S…

2019 The Astrophysical Journal
IRIS 40
The MASSIVE Survey. XII. Connecting Stellar Populations of Early-type Galaxies to Kinematics and Environment
DOI: 10.3847/1538-4357/ab01e3 Bibcode: 2019ApJ...874...66G

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +6 more

We measure the stellar populations as a function of the radius for 90 early-type galaxies (ETGs) in the MASSIVE survey, a volume-limited integral-field spectroscopic (IFS) galaxy survey targeting all northern-sky ETGs with an absolute K-band magnitude of M K < -25.3 mag or a stellar mass of {M}* ≳ 4× {10}11 {M…

2019 The Astrophysical Journal
eHST 40
Carbon-rich (DQ) white dwarfs in the Sloan Digital Sky Survey
DOI: 10.1051/0004-6361/201935946 Bibcode: 2019A&A...628A.102K

Kepler, S. O.; Koester, D.

Context. Among the spectroscopically identified white dwarfs, a fraction smaller than 2% have spectra dominated by carbon lines, mainly molecular C2, but also a smaller group dominated by C I and C II lines. These are together called DQ white dwarfs.
Aims: We want to derive atmospheric parameters Teff, log g, and carbon …

2019 Astronomy and Astrophysics
Gaia 40