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A unique hot Jupiter spectral sequence with evidence for compositional diversity
DOI: 10.1038/s41550-021-01455-4 Bibcode: 2021NatAs...5.1224M

Fortney, Jonathan J.; Sing, David K.; López-Morales, Mercedes +11 more

The emergent spectra of close-in, giant exoplanets (`hot Jupiters') are expected to be distinct from those of self-luminous objects with similar effective temperatures because hot Jupiters are primarily heated from above by their host stars rather than internally from the release of energy from their formation1. Theoretical models predi…

2021 Nature Astronomy
eHST 67
BAT AGN Spectroscopic Survey. XX. Molecular Gas in Nearby Hard-X-Ray-selected AGN Galaxies
DOI: 10.3847/1538-4365/abcbfe Bibcode: 2021ApJS..252...29K

Lamperti, Isabella; Schawinski, Kevin; Saintonge, Amelie +23 more

We present the host-galaxy molecular gas properties of a sample of 213 nearby (0.01 < z < 0.05) hard-X-ray-selected active galactic nucleus (AGN) galaxies, drawn from the 70-month catalog of Swift's Burst Alert Telescope (BAT), with 200 new CO(2-1) line measurements obtained with the James Clerk Maxwell Telescope and the Atacama Pathfinder E…

2021 The Astrophysical Journal Supplement Series
Herschel 67
Detection and Bulk Properties of the HR 8799 Planets with High-resolution Spectroscopy
DOI: 10.3847/1538-3881/ac1349 Bibcode: 2021AJ....162..148W

Knutson, Heather; Duchêne, Gaspard; Fitzgerald, Michael P. +49 more

Using the Keck Planet Imager and Characterizer, we obtained high-resolution (R ~ 35,000) K-band spectra of the four planets orbiting HR 8799. We clearly detected H2O and CO in the atmospheres of HR 8799 c, d, and e, and tentatively detected a combination of CO and H2O in b. These are the most challenging directly imaged exopl…

2021 The Astronomical Journal
Gaia 67
Self-consistent Stellar Radial Velocities from LAMOST Medium-resolution Survey DR7
DOI: 10.3847/1538-4365/ac0834 Bibcode: 2021ApJS..256...14Z

Tian, Hao; Zong, Weikai; Fu, Jian-Ning +12 more

Radial velocity (RV) is among the most fundamental physical quantities obtainable from stellar spectra and is rather important in the analysis of time-domain phenomena. LAMOST Medium-resolution Survey (MRS) DR7 contains five million single-exposure stellar spectra with spectral resolution R ~ 7500. However, the temporal variation of the RV zero-po…

2021 The Astrophysical Journal Supplement Series
Gaia 67
New insight into the magnetism of degenerate stars from the analysis of a volume-limited sample of white dwarfs
DOI: 10.1093/mnras/stab2046 Bibcode: 2021MNRAS.507.5902B

Bagnulo, S.; Landstreet, J. D.

Many stars evolve into magnetic white dwarfs (MWDs), and observations may help to understand when the magnetic field appears at the stellar surface, if and how it evolves during the cooling phase, and, above all, what are the mechanisms that generate it. After obtaining new spectropolarimetric observations and combining them with previous literatu…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 67
Tree-ring structure of Galactic bar resonance
DOI: 10.1093/mnras/stab1094 Bibcode: 2021MNRAS.505.2412C

Schönrich, Ralph; Chiba, Rimpei

Galaxy models have long predicted that galactic bars slow down by losing angular momentum to their postulated dark haloes. When the bar slows down, resonance sweeps radially outwards through the galactic disc while growing in volume, thereby sequentially capturing new stars at its surface/separatrix. Since trapped stars conserve their action of li…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 66
Radii of young star clusters in nearby galaxies
DOI: 10.1093/mnras/stab2907 Bibcode: 2021MNRAS.508.5935B

Gnedin, Oleg Y.; Brown, Gillen

We measure the projected half-light radii of young star clusters in 31 galaxies from the Legacy Extragalactic UV Survey (LEGUS). We implement a custom pipeline specifically designed to be robust against contamination, which allows us to measure radii for 6097 clusters. This is the largest sample of young star cluster radii currently available. We …

2021 Monthly Notices of the Royal Astronomical Society
eHST 66
Validation of the accuracy and precision of Gaia EDR3 parallaxes with globular clusters
DOI: 10.1051/0004-6361/202140418 Bibcode: 2021A&A...649A..13M

Maíz Apellániz, J.; Barbá, R. H.; Pantaleoni González, M.

Context. The recent early third data release (EDR3) from the Gaia mission has produced parallaxes for 1.468 × 109 sources with better quality than those reported in the previous data release. Nevertheless, there are calibration issues with the data that require corrections to the published values and uncertainties.
Aims: We want to…

2021 Astronomy and Astrophysics
Gaia 66
The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance
DOI: 10.3847/1538-3881/ac082a Bibcode: 2021AJ....162..176P

Gies, Douglas R.; Quinn, Samuel N.; Henry, Todd J. +5 more

We report initial results of a large radial velocity survey of K dwarfs up to a distance of 50 pc from the solar system, to look for stellar, brown dwarf, and Jovian planets using radial velocities from the CHIRON spectrograph on the CTIO/SMARTS 1.5 m telescope. We identify three new exoplanet candidates orbiting host stars in the K dwarf survey a…

2021 The Astronomical Journal
Gaia 66
Magnetohydrodynamic Waves in Open Coronal Structures
DOI: 10.1007/s11214-021-00849-0 Bibcode: 2021SSRv..217...76B

Tian, H.; Wang, T. J.; Banerjee, D. +8 more

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic waves in the solar corona. The propagating waves (in contrast to the standing waves) are usually originated in the lower solar atmosphere which makes them particularly relevant to coronal heating. Furthermore, open coronal structures are believed to be the source reg…

2021 Space Science Reviews
IRIS 66