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Modeling the mixed-morphology supernova remnant IC 443. Origins of its complex morphology and X-ray emission
DOI: 10.1051/0004-6361/202039940 Bibcode: 2021A&A...649A..14U

Miceli, M.; Bocchino, F.; Orlando, S. +4 more

Context. The morphology and the distribution of material observed in supernova remnants (SNRs) reflect the interaction of the supernova (SN) blast wave with the ambient environment, the physical processes associated with the SN explosion, and the internal structure of the progenitor star. IC 443 is a mixed-morphology (MM) SNR located in a quite co…

2021 Astronomy and Astrophysics
XMM-Newton 24
STIX X-ray microflare observations during the Solar Orbiter commissioning phase
DOI: 10.1051/0004-6361/202140524 Bibcode: 2021A&A...656A...4B

Massa, Paolo; Krucker, Säm; Piana, Michele +34 more

Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is the hard X-ray instrument onboard Solar Orbiter designed to observe solar flares over a broad range of flare sizes.
Aims: We report the first STIX observations of solar microflares recorded during the instrument commissioning phase in order to investigate the STIX performance at…

2021 Astronomy and Astrophysics
Hinode SolarOrbiter 24
Phase-curve Pollution of Exoplanet Transmission Spectra
DOI: 10.3847/1538-3881/abe048 Bibcode: 2021AJ....161..174M

Lagage, Pierre-Olivier; Morello, Giuseppe; Zingales, Tiziano +2 more

The occurrence of a planet transiting in front of its host star offers the opportunity to observe the planet's atmosphere filtering starlight. The fraction of occulted stellar flux is roughly proportional to the optically thick area of the planet, the extent of which depends on the opacity of the planet's gaseous envelope at the observed wavelengt…

2021 The Astronomical Journal
Gaia eHST 24
Machine learning initialization to accelerate Stokes profile inversions
DOI: 10.1051/0004-6361/201936910 Bibcode: 2021A&A...651A..31G

Ruiz Cobo, B.; Quintero Noda, C.; Orozco Suárez, D. +3 more

Context. At present, an exponential growth in scientific data from current and upcoming solar observatories is expected. Most of the data consist of high spatial and temporal resolution cubes of Stokes profiles taken in both local thermodynamic equilibrium (LTE) and non-LTE spectral lines. The analysis of such solar observations requires complex i…

2021 Astronomy and Astrophysics
Hinode 24
Black hole mass measurement using ALMA observations of [CI] and CO emissions in the Seyfert 1 galaxy NGC 7469
DOI: 10.1093/mnras/stab1002 Bibcode: 2021MNRAS.504.4123N

Baba, Shunsuke; Meier, David S.; Turner, Jean L. +11 more

We present a supermassive black hole (SMBH) mass measurement in the Seyfert 1 galaxy NGC 7469 using Atacama Large Millimeter/submillimeter Array (ALMA) observations of the atomic-[CI](1-0) and molecular-12CO(1-0) emission lines at the spatial resolution of ≈0${_{.}^{\prime\prime}}$3 (or ≈100 pc). These emissions reveal that NGC 7469 hos…

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Detected in a Solar Eruption
DOI: 10.1007/s11207-021-01913-2 Bibcode: 2021SoPh..296..169Z

Shen, Yuandeng; Zhou, Chengrui; Zhou, Xinping +4 more

We present Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observation of three types of fast-mode, propagating, magnetosonic waves in a GOES C3.0 flare on 23 April 2013, which was accompanied by a prominence eruption and a broad coronal mass ejection (CME). During the fast-rising phase of the prominence, a large-scale, dome-shap…

2021 Solar Physics
SOHO 24
NICER Detection of Thermal X-Ray Pulsations from the Massive Millisecond Pulsars PSR J0740+6620 and PSR J1614-2230
DOI: 10.3847/2041-8213/ac158e Bibcode: 2021ApJ...918L..26W

Bogdanov, Slavko; Ray, Paul S.; Wolff, Michael T. +11 more

We report the detection of X-ray pulsations from the rotation-powered millisecond-period pulsars PSR J0740+6620 and PSR J1614-2230, two of the most massive neutron stars known, using observations with the Neutron Star Interior Composition Explorer (NICER). We also analyze X-ray Multi-Mirror Mission (XMM-Newton) data for both pulsars to obtain thei…

2021 The Astrophysical Journal
XMM-Newton 24
Science Highlights and Final Updates from 17 Years of Total Solar Irradiance Measurements from the SOlar Radiation and Climate Experiment/Total Irradiance Monitor (SORCE/TIM)
DOI: 10.1007/s11207-021-01853-x Bibcode: 2021SoPh..296..133K

Kopp, Greg

The final version (V.19) of the total solar irradiance data from the SOlar Radiation and Climate Experiment (SORCE) Total Irradiance Monitor has been released. This version includes all calibrations updated to the end of the mission and provides irradiance data from 25 February 2003 through 25 February 2020. These final calibrations are presented …

2021 Solar Physics
SOHO 24
Filament Rotation in the California L1482 Cloud
DOI: 10.3847/1538-4357/abd47c Bibcode: 2021ApJ...908...86A

Klessen, R. S.; Stutz, A. M.; Law, C. Y. +5 more

We analyze the gas mass distribution, the gas kinematics, and the young stellar objects of the California Molecular Cloud L1482 filament. The mean Gaia DR2 YSO distance is ${511}_{-16}^{+17}$ pc. In terms of the gas, the line-mass (M/L) profiles are symmetric scale-free power laws consistent with cylindrical geometry. We calculate the gravitationa…

2021 The Astrophysical Journal
Gaia Herschel 24
Ancient Very Metal-poor Stars Associated with the Galactic Disk in the H3 Survey
DOI: 10.3847/1538-4357/abcda4 Bibcode: 2021ApJ...908..208C

Conroy, Charlie; Ting, Yuan-Sen; Cargile, Phillip A. +8 more

Ancient, very metal-poor (VMP) stars offer a window into the earliest epochs of galaxy formation and assembly. We combine data from the H3 Spectroscopic Survey and Gaia to measure metallicities, abundances of α elements, stellar ages, and orbital properties of a sample of 482 VMP ([Fe/H] < -2) stars in order to constrain their origins. This sam…

2021 The Astrophysical Journal
Gaia 24