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Steady-state nucleosynthesis throughout the Galaxy
DOI: 10.1016/j.newar.2020.101608 Bibcode: 2021NewAR..9201608D

Wang, Wei; Martin, Pierrick; Diehl, Roland +6 more

The measurement and astrophysical interpretation of characteristic γ-ray lines from nucleosynthesis was one of the prominent science goals of the INTEGRAL mission and in particular its spectrometer SPI. Emission from 26Al and from 60Fe decay lines, due to their My decay times, originates from accumulated ejecta of nucleosynth…

2021 New Astronomy Reviews
INTEGRAL 12
The Dayside Ionopause of Mars: Solar Wind Interaction, Pressure Balance, and Comparisons With Venus
DOI: 10.1029/2021JE006936 Bibcode: 2021JGRE..12606936C

Gurnett, D. A.; Kopf, A. J.; Halekas, J. +5 more

Due to the lower ionospheric thermal pressure and existence of the crustal magnetism at Mars, the Martian ionopause is expected to behave differently from the ionopause at Venus. We study the solar wind interaction and pressure balance at the ionopause of Mars using both in situ and remote sounding measurements from the Mars Advanced Radar for Sub…

2021 Journal of Geophysical Research (Planets)
MEx 12
The Swan: Data-driven Inference of Stellar Surface Gravities for Cool Stars from Photometric Light Curves
DOI: 10.3847/1538-3881/abdf4c Bibcode: 2021AJ....161..170S

Huber, Daniel; Ness, Melissa K.; Wheeler, Adam +1 more

Stellar light curves are well known to encode physical stellar properties. Precise, automated, and computationally inexpensive methods to derive physical parameters from light curves are needed to cope with the large influx of these data from space-based missions such as Kepler and TESS. Here we present a new methodology that we call "The Swan," a…

2021 The Astronomical Journal
Gaia 12
A synergy of the velocity gradients technique and the probability density functions for identifying gravitational collapse in self-absorbing media
DOI: 10.1093/mnras/stab087 Bibcode: 2021MNRAS.502.1768H

Lazarian, A.; Hu, Yue

The velocity gradients technique (VGT) and the probability density functions (PDFs) of mass density are tools to study turbulence, magnetic fields, and self-gravity in molecular clouds. However, self-absorption can significantly make the observed intensity different from the column density structures. In this work, we study the effects of self-abs…

2021 Monthly Notices of the Royal Astronomical Society
Herschel 12
A 99 minute Double-lined White Dwarf Binary from SDSS-V
DOI: 10.3847/1538-4357/ac2145 Bibcode: 2021ApJ...921..160C

Maoz, Dan; Hermes, J. J.; Rix, Hans-Walter +12 more

We report the discovery of SDSS J133725.26+395237.7 (hereafter SDSS J1337+3952), a double-lined white dwarf (WD+WD) binary identified in early data from the fifth-generation Sloan Digital Sky Survey (SDSS-V). The double-lined nature of the system enables us to fully determine its orbital and stellar parameters with follow-up Gemini spectroscopy an…

2021 The Astrophysical Journal
Gaia 12
Radius and Mass Distribution of Ultra-short-period Planets
DOI: 10.3847/1538-4357/ac0bb8 Bibcode: 2021ApJ...919...26U

Uzsoy, Ana Sofía M.; Rogers, Leslie A.; Price, Ellen M.

Ultra-short-period (USP) planets are an enigmatic subset of exoplanets defined by having orbital periods <1 day. It is still not understood how USP planets form, or to what degree they differ from planets with longer orbital periods. Most USP planets have radii <2 R, while planets that orbit further from their star extend to Jupi…

2021 The Astrophysical Journal
Gaia 12
Radio Counterpart Candidates to Unassociated 4FGL-DR2 Sources
DOI: 10.3847/1538-4357/abf73b Bibcode: 2021ApJ...914...42B

Schinzel, F. K.; Bruzewski, S.; Taylor, G. B. +1 more

For the duration of the Fermi Gamma-Ray Space Telescope's mission, approximately one-third of the point sources detected have been noted as "unassociated," meaning that they seem to have no known counterpart at any other wavelength/frequency. This mysterious part of the gamma-ray sky is perhaps one of the largest unknowns in current astronomical p…

2021 The Astrophysical Journal
Gaia 12
A transmission spectrum of the planet candidate WD 1856+534 b and a lower limit to its mass
DOI: 10.1051/0004-6361/202140359 Bibcode: 2021A&A...649A.131A

Alonso, R.; Hollands, M. A.; Castro-Rodríguez, N. +7 more

The cool white dwarf WD 1856+534 was found to be transited by a Jupiter-sized object with a mass at or below 14 MJup. We used the GTC telescope to obtain and analyse the photometry and low-resolution spectroscopy of six transits of WD 1856+534 b, with the intention of deriving the slope of the transmission spectrum. Such a slope, assumi…

2021 Astronomy and Astrophysics
Gaia 12
Solar wind rotation rate and shear at coronal hole boundaries. Possible consequences for magnetic field inversions
DOI: 10.1051/0004-6361/202040180 Bibcode: 2021A&A...653A..92P

Lavraud, B.; Fargette, N.; Rouillard, A. P. +6 more

Context. In situ measurements by several spacecraft have revealed that the solar wind is frequently perturbed by transient structures that have been interpreted as magnetic folds, jets, waves, and flux ropes that propagate rapidly away from the Sun over a large range of heliocentric distances. Parker Solar Probe (PSP), in particular, has detected …

2021 Astronomy and Astrophysics
SOHO 12
One Source, Two Source(s): Ribs and Tethers
DOI: 10.3390/galaxies9040081 Bibcode: 2021Galax...9...81R

Knowles, Kenda; Rudnick, Lawrence; Kolokythas, Konstantinos +1 more

We present the unique and challenging case of a radio galaxy in Abell 3266 observed as part of the MeerKAT Galaxy Cluster Legacy Survey. It has quasi-periodic bright patches along the tail which connect to never-before-seen thin transverse extensions, which we call "ribs", reaching up to ∼50 kpc from the central axis of the tail. At a distance of …

2021 Galaxies
XMM-Newton 12