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A cool and inflated progenitor candidate for the Type Ib supernova 2019yvr at 2.6 yr before explosion
DOI: 10.1093/mnras/stab838 Bibcode: 2021MNRAS.504.2073K

Kilpatrick, Charles D.; Drout, Maria R.; Foley, Ryan J. +13 more

We present Hubble Space Telescope imaging of a pre-explosion counterpart to SN 2019yvr obtained 2.6 yr before its explosion as a type Ib supernova (SN Ib). Aligning to a post-explosion Gemini-S/GSAOI image, we demonstrate that there is a single source consistent with being the SN 2019yvr progenitor system, the second SN Ib progenitor candidate aft…

2021 Monthly Notices of the Royal Astronomical Society
eHST 76
Investigating the young AU Mic system with SPIRou: large-scale stellar magnetic field and close-in planet mass
DOI: 10.1093/mnras/staa3702 Bibcode: 2021MNRAS.502..188K

Gaidos, Eric; Doyon, René; Donati, Jean-François +12 more

We present a velocimetric and spectropolarimetric analysis of 27 observations of the 22-Myr M1 star AU Microscopii (AU Mic) collected with the high-resolution YJHK (0.98-2.35 µm) spectropolarimeter SPIRou from 2019 September 18 to November 14. Our radial velocity (RV) time-series exhibits activity-induced fluctuations of 45 m s-1

2021 Monthly Notices of the Royal Astronomical Society
Gaia 76
APOGEE DR16: A multi-zone chemical evolution model for the Galactic disc based on MCMC methods
DOI: 10.1051/0004-6361/202039864 Bibcode: 2021A&A...647A..73S

Calura, F.; Palla, M.; Matteucci, F. +6 more

Context. The analysis of the latest release of the Apache Point Observatory Galactic Evolution Experiment project (APOGEE DR16) data suggests the existence of a clear distinction between two sequences of disc stars at different Galactocentric distances in the [α/Fe] versus [Fe/H] abundance ratio space: the so-called high-α sequence, classically as…

2021 Astronomy and Astrophysics
Gaia 76
The Hi-GAL compact source catalogue - II. The 360° catalogue of clump physical properties
DOI: 10.1093/mnras/stab1038 Bibcode: 2021MNRAS.504.2742E

Martin, P. G.; Paladini, R.; Pilbratt, G. L. +29 more

We present the 360° catalogue of physical properties of Hi-GAL compact sources, detected between 70 and 500 $\mu$m. This release not only completes the analogous catalogue previously produced by the Hi-GAL collaboration for -71° ≲ ℓ ≲ 67°, but also meaningfully improves it because of a new set of heliocentric distances, 120 808 in total. About a t…

2021 Monthly Notices of the Royal Astronomical Society
Herschel 76
Primordial black holes and scalar-induced secondary gravitational waves from inflationary models with a noncanonical kinetic term
DOI: 10.1103/PhysRevD.103.063534 Bibcode: 2021PhRvD.103f3534Y

Gao, Qing; Gong, Yungui; Yi, Zhu +1 more

With the enhancement mechanism provided by a noncanonical kinetic term with a peak, the amplitude of primordial curvature perturbations can be enhanced by seven orders of magnitude at small scales while keeping to be consistent with observations at large scales. The peak function and inflationary potential are not restricted in this mechanism. We …

2021 Physical Review D
INTEGRAL 76
Turbulent Gas in Lensed Planck-selected Starbursts at z ∼ 1-3.5
DOI: 10.3847/1538-4357/abcc01 Bibcode: 2021ApJ...908...95H

Frayer, D. T.; Frye, B. L.; Jiménez-Andrade, E. F. +26 more

Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the universe. Key aspects to these processes are the gas heating and cooling mechanisms, and although it is well known that these galaxies are gas-rich, little is known about the gas excitation conditions. Only a few detailed radiative…

2021 The Astrophysical Journal
Herschel 76
Extending the evolution of the stellar mass-size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS
DOI: 10.1093/mnras/stab1744 Bibcode: 2021MNRAS.506..928N

Ferguson, Henry C.; Kartaltepe, Jeyhan S.; Martis, Nicholas S. +23 more

We reliably extend the stellar mass-size relation over 0.2 ≤ z ≤ 2 to low stellar mass galaxies by combining the depth of Hubble Frontier Fields with the large volume covered by CANDELS. Galaxies are simultaneously modelled in multiple bands using the tools developed by the MegaMorph project, allowing robust size (i.e. half-light radius) estimates…

2021 Monthly Notices of the Royal Astronomical Society
eHST 75
Validation of the Gaia Early Data Release 3 Parallax Zero-point Model with Asteroseismology
DOI: 10.3847/1538-3881/abe936 Bibcode: 2021AJ....161..214Z

Zinn, Joel C.

Gaia Early Data Release 3 (EDR3) provides trigonometric parallaxes for 1.5 billion stars, with reduced systematics compared to Gaia Data Release 2 and reported precisions better by up to a factor of 2. New to EDR3 is a tentative model for correcting the parallaxes of magnitude-, position-, and color-dependent systematics for five- and six-paramete…

2021 The Astronomical Journal
Gaia 75
Elevated r-process Enrichment in Gaia Sausage and Sequoia
DOI: 10.3847/2041-8213/abdbb8 Bibcode: 2021ApJ...908L...8A

Myeong, G. C.; Kobayashi, Chiaki; Belokurov, Vasily +6 more

The Gaia Sausage (GS) and the Sequoia represent the major accretion events that formed the stellar halo of the Milky Way. A detailed chemical study of these main building blocks provides a pristine view of the early steps of the Galaxy's assembly. We present the results of the analysis of the UVES high-resolution spectroscopic observations at the …

2021 The Astrophysical Journal
Gaia 75
Solar force-free magnetic fields
DOI: 10.1007/s41116-020-00027-4 Bibcode: 2021LRSP...18....1W

Wiegelmann, Thomas; Sakurai, Takashi

The structure and dynamics of the solar corona is dominated by the magnetic field. In most areas in the corona magnetic forces are so dominant that all non-magnetic forces such as plasma pressure gradients and gravity can be neglected in the lowest order. This model assumption is called the force-free field assumption, as the Lorentz force vanishe…

2021 Living Reviews in Solar Physics
Hinode 75