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Composite bulges - II. Classical bulges and nuclear discs in barred galaxies: the contrasting cases of NGC 4608 and NGC 4643
DOI: 10.1093/mnras/stab126 Bibcode: 2021MNRAS.502.2446E

Beckman, John E.; Bender, Ralf; Drory, Niv +14 more

We present detailed morphological, photometric, and stellar-kinematic analyses of the central regions of two massive, early-type barred galaxies with nearly identical large-scale morphologies. Both have large, strong bars with prominent inner photometric excesses that we associate with boxy/peanut-shaped (B/P) bulges; the latter constitute ∼30 per…

2021 Monthly Notices of the Royal Astronomical Society
eHST 21
The magnetic field across the molecular warped disk of Centaurus A
DOI: 10.1038/s41550-021-01329-9 Bibcode: 2021NatAs...5..604L

Lopez-Rodriguez, Enrique

Magnetic fields are amplified as a consequence of galaxy formation and turbulence-driven dynamos. Galaxy mergers can potentially amplify the magnetic fields from their progenitors, making the magnetic fields dynamically important. However, the effect of mergers on magnetic fields is still poorly understood. We use thermal polarized emission observ…

2021 Nature Astronomy
Herschel 21
The Dark World: A Tale of WASP-43b in Reflected Light with HST WFC3/UVIS
DOI: 10.3847/1538-3881/abe8d6 Bibcode: 2021AJ....161..269F

Fortney, Jonathan J.; Stevenson, Kevin B.; Mayorga, L. C. +14 more

Optical reflected light eclipse observations provide a direct probe of exoplanet scattering properties, such as from aerosols. We present here the photometric reflected light observations of WASP-43b using the Hubble Space Telescope (HST) WFC3/UVIS instrument with the F350LP filter (346-822 nm) encompassing the entire optical band. This is the fir…

2021 The Astronomical Journal
eHST 21
XMMU J050722.1-684758: discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847
DOI: 10.1093/mnras/stab716 Bibcode: 2021MNRAS.504..326M

Haberl, F.; Udalski, A.; Filipović, M. D. +5 more

We report the discovery of a new high-mass X-ray binary pulsar, XMMU J050722.1-684758, possibly associated with the supernova remnant (SNR) MCSNR J0507-6847 in the Large Magellanic Cloud, using XMM-NewtonX-ray observations. Pulsations with a periodicity of 570 s are discovered from the Be X-ray binary XMMU J050722.1-684758 confirming its nature as…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 21
The Anatomy of an Unusual Edge-on Protoplanetary Disk. I. Dust Settling in a Cold Disk
DOI: 10.3847/1538-3881/abeb1d Bibcode: 2021AJ....161..238W

Duchêne, Gaspard; Wolff, Schuyler G.; Perrin, Marshall D. +7 more

As the earliest stage of planet formation, massive, optically thick, and gas-rich protoplanetary disks provide key insights into the physics of star and planet formation. When viewed edge-on, high-resolution images offer a unique opportunity to study both the radial and vertical structures of these disks and relate this to vertical settling, radia…

2021 The Astronomical Journal
eHST 21
Masses of White Dwarf Binary Companions to Type Ia Supernovae Measured from Runaway Velocities
DOI: 10.3847/2041-8213/ac432d Bibcode: 2021ApJ...923L..34B

Hermes, J. J.; Shen, Ken J.; Chandra, Vedant +1 more

The recently proposed "dynamically driven double-degenerate double-detonation" (D6) scenario posits that Type Ia supernovae (SNe) may occur during dynamically unstable mass transfer between two white dwarfs (WDs) in a binary. This scenario predicts that the donor WD may then survive the explosion and be released as a hypervelocity runaw…

2021 The Astrophysical Journal
Gaia 21
A New Catalog of Asymptotic Giant Branch Stars in Our Galaxy
DOI: 10.3847/1538-4365/ac1274 Bibcode: 2021ApJS..256...43S

Suh, Kyung-Won

We present a new catalog of 11,209 O-rich asymptotic giant branch (AGB) stars and 7172 C-rich AGB stars in our Galaxy, identifying more AGB stars in the bulge component and considering more visual carbon stars. For each object, we cross-identify the Infrared Astronomical Satellite (IRAS), AKARI, Midcourse Space Experiment, Wide-field Infrared Surv…

2021 The Astrophysical Journal Supplement Series
AKARI 21
Sixty Years of Element Abundance Measurements in Solar Energetic Particles
DOI: 10.1007/s11214-021-00845-4 Bibcode: 2021SSRv..217...72R

Reames, Donald V.

Sixty years ago the first observation was published showing solar energetic particles (SEPs) with a sampling of chemical elements with atomic numbers 6 ≤Z ≤18 above 40 MeV amu−1. Thus began study of the direct products of dynamic physics in the solar corona. As we have progressed from 4-min sounding-rocket samples to continuous satellit…

2021 Space Science Reviews
Ulysses 21
BALRoGO: Bayesian Astrometric Likelihood Recovery of Galactic Objects - Global properties of over one hundred globular clusters with Gaia EDR3
DOI: 10.1093/mnras/stab947 Bibcode: 2021MNRAS.504.1355V

Vitral, Eduardo

We present BALRoGO: Bayesian Astrometric Likelihood Recovery of Galactic Objects, a public code to measure the centres, effective radii, and bulk proper motions of Milky Way (MW) globular clusters and Local Group dwarf spheroidals, whose data are mixed with MW field stars. Our approach presents innovative methods such as surface density fits allow…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 21
First dust measurements with the Solar Orbiter Radio and Plasma Wave instrument
DOI: 10.1051/0004-6361/202140969 Bibcode: 2021A&A...656A..30Z

Maksimovic, M.; Bale, S. D.; Chust, T. +20 more

Context. Impacts of dust grains on spacecraft are known to produce typical impulsive signals in the voltage waveform recorded at the terminals of electric antennas. Such signals (as may be expected) are routinely detected by the Time Domain Sampler (TDS) system of the Radio and Plasma Waves (RPW) instrument on board Solar Orbiter.
Aims: We in…

2021 Astronomy and Astrophysics
SolarOrbiter 21