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Fast Reconstruction of 3D Density Distribution around the Sun Based on the MAS by Deep Learning
DOI: 10.3847/1538-4357/acbd3c Bibcode: 2023ApJ...948...21R

Moon, Yong-Jae; Rahman, Sumiaya; Park, Eunsu +5 more

This study is the first attempt to generate a three-dimensional (3D) coronal electron density distribution based on the pix2pixHD model, whose computing time is much shorter than that of the magnetohydrodynamic (MHD) simulation. For this, we consider photospheric solar magnetic fields as input, and electron density distribution simulated with the …

2023 The Astrophysical Journal
SOHO 5
Detection of optical emission from the supernova remnant G7.7-3.7
DOI: 10.1093/mnras/stad2779 Bibcode: 2023MNRAS.526.1112D

Boumis, P.; Vink, J.; Chiotellis, A. +6 more

We present the first optical study of the supernova remnant (SNR) G7.7-3.7, with the aim of determining its evolutionary phase since it has been suggested to be the remnant of SN 386 AD. We obtained narrow-band images in the filters H α + [N II], H β, [O III], [S II] that revealed faint optical emission in the southern region of the SNR consisting…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Independent Validation of the Temperate Super-Earth HD 79211 b using HARPS-N
DOI: 10.3847/1538-3881/ac9ccd Bibcode: 2023AJ....165...38D

López-Morales, Mercedes; Bieryla, Allyson; Stassun, Keivan G. +28 more

We present high-precision radial velocities (RVs) from the HARPS-N spectrograph for HD 79210 and HD 79211, two M0V members of a gravitationally bound binary system. We detect a planet candidate with a period of ${24.421}_{-0.017}^{+0.016}$ days around HD 79211 in these HARPS-N RVs, validating the planet candidate originally identified in CARMENES …

2023 The Astronomical Journal
Gaia 5
Dense Molecular Environments of B[e] Supergiants and Yellow Hypergiants
DOI: 10.3390/galaxies11030076 Bibcode: 2023Galax..11...76K

Kraus, Michaela; Torres, Andrea F.; Kourniotis, Michalis +2 more

Massive stars expel large amounts of mass during their late evolutionary phases. We aim to unveil the physical conditions within the warm molecular environments of B[e] supergiants (B[e]SGs) and yellow hypergiants (YHGs), which are known to be embedded in circumstellar shells and disks. We present K-band spectra of two B[e]SGs from the Large Magel…

2023 Galaxies
Gaia 5
Electrostatic Solitary Waves in the Venusian Ionosphere Pervaded by the Solar Wind: A Theoretical Perspective
DOI: 10.3847/1538-4357/acd2d7 Bibcode: 2023ApJ...950..111R

Lakhina, G. S.; Kamalam, T.; Singh, S. V. +3 more

Electrostatic solitary waves (ESWs) in the Venusian ionosphere that are impinged by the solar wind are investigated using a homogeneous, collisionless, and magnetized multicomponent plasma consisting of Venusian H+ and O+ ions, Maxwellian Venusian electrons and streaming solar wind protons, and suprathermal electrons followin…

2023 The Astrophysical Journal
SolarOrbiter 5
Observed dust surface density across cosmic times
DOI: 10.1093/mnras/stad1235 Bibcode: 2023MNRAS.522.4852P

Howk, J. Christopher; Péroux, Céline; De Cia, Annalisa

Our ability to interpret observations of galaxies and trace their stellar, gas, and dust content over cosmic time critically relies on our understanding of how the dust abundance and properties vary with environment. Here, we compute the dust surface density across cosmic times to put novel constraints on simulations of the build-up of dust. We pr…

2023 Monthly Notices of the Royal Astronomical Society
eHST 5
The ultraluminous X-ray source M 81 X-6: a weakly magnetised neutron star with a precessing accretion disc?
DOI: 10.1051/0004-6361/202244576 Bibcode: 2023A&A...669A.130A

Godet, O.; Webb, N. A.; Middleton, M. J. +2 more

Context. Thanks to their proximity, ultraluminous X-ray sources (ULXs) represent a privileged astrophysical laboratory to study super-Eddington accretion. Current open questions concern the nature of the compact object, which is still hard to determine in those cases where pulsations are not directly detected, and the mechanisms responsible for th…

2023 Astronomy and Astrophysics
XMM-Newton 5
Halfway to the Peak: Spatially Resolved Star Formation and Kinematics in a z = 0.54 Dusty Galaxy with JWST/MIRI
DOI: 10.3847/2041-8213/ad07e1 Bibcode: 2023ApJ...958L...5Y

Veilleux, Sylvain; Ogle, Patrick; Alberts, Stacey +16 more

We present JWST Mid-InfraRed Instrument/Medium-Resolution Spectrometer (MIRI/MRS) observations of an infrared luminous disk galaxy, FLS1, at z ~ 0.54. With a lookback time of 5 Gyr, FLS1 is chronologically at the midpoint between the peak epoch of star formation and the present day. The MRS data provide maps of the atomic fine structure lines [Ar …

2023 The Astrophysical Journal
ISO eHST JWST 5
Separated Twins or Just Siblings? A Multiplanet System around an M Dwarf Including a Cool Sub-Neptune
DOI: 10.3847/2041-8213/ad037d Bibcode: 2023ApJ...959L...1H

Quinn, Samuel N.; Stassun, Keivan G.; Zhou, George +27 more

We report the discovery of two TESS sub-Neptunes orbiting the early M dwarf TOI-904 (TIC 261257684). Both exoplanets, TOI-904 b and c, were initially observed in TESS Sector 12 with twin sizes of ${2.426}_{-0.157}^{+0.163}$ and ${2.167}_{-0.118}^{+0.130}$ R , respectively. Through observations in five additional sectors in the TESS pri…

2023 The Astrophysical Journal
Gaia 5
Orbits and Masses of the Small Satellites of Pluto
DOI: 10.3847/PSJ/acde77 Bibcode: 2023PSJ.....4..120P

Porter, Simon B.; Canup, Robin M.

We present a new orbit and mass solution for the four small satellites of Pluto: Styx, Nix, Kerberos, and Hydra. We have reanalyzed all available observations of the Pluto system obtained by the Hubble Space Telescope from 2005 to 2019 with the ACS, WFPC2, and WFC3 instruments, as well as the New Horizons LORRI images taken on approach to Pluto in…

2023 The Planetary Science Journal
eHST 5