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The Fengyun-3E/Joint Total Solar Irradiance Absolute Radiometer: Instrument Design, Characterization, and Calibration
DOI: 10.1007/s11207-021-01794-5 Bibcode: 2021SoPh..296...52S

Zhao, Yan; Fang, Wei; Finsterle, Wolfgang +6 more

The Joint Total Solar Irradiance Monitor (JTSIM) is due to fly onboard the Fengyun-3E spacecraft and aims to measure the Total Solar Irradiance (TSI) in orbit. The instruments on the Fengyun-3E/JTSIM include the Digital Absolute Radiometer (DARA) from the Physikalisch Meteorologisches Observatorium, Davos and World Radiation Center (PMOD/WRC) and …

2021 Solar Physics
SOHO 5
Pre-explosion Properties of Helium Star Donors to Thermonuclear Supernovae
DOI: 10.3847/1538-4357/ac27ae Bibcode: 2021ApJ...922..241W

Schwab, Josiah; Götberg, Ylva; Wong, Tin Long Sunny

Helium star-carbon-oxygen white dwarf (CO WD) binaries are potential single-degenerate progenitor systems of thermonuclear supernovae. Revisiting a set of binary evolution calculations using the stellar evolution code MESA, we refine our previous predictions about which systems can lead to a thermonuclear supernova and then characterize the proper…

2021 The Astrophysical Journal
eHST 5
Multiple Stellar Populations at Less-evolved Stages-II: No Evidence of Significant Helium Spread among NGC 1846 Dwarfs
DOI: 10.3847/1538-4357/ac2059 Bibcode: 2021ApJ...921..171L

Li, Chengyuan

The detection of star-to-star chemical variations in star clusters older than 2 Gyr has changed the traditional view of star clusters as canonical examples of "simple stellar populations" into the so-called "multiple stellar populations" (MPs). Although the significance of MPs seems to correlate with cluster total mass, it seems that the presence …

2021 The Astrophysical Journal
eHST 5
A new search for star forming regions in the southern outer Galaxy
DOI: 10.1051/0004-6361/202039523 Bibcode: 2021A&A...645A.113K

König, C.; Menten, K. M.; Wyrowski, F. +2 more

Context. Star formation in the outer Galaxy is thought to be different from that in the inner Galaxy, as it is subject to different environmental parameters such as metallicity, interstellar radiation field, or mass surface density, which all change with galactocentric radius. Extending our star formation knowledge, from the inner to the outer Gal…

2021 Astronomy and Astrophysics
Herschel 5
X-ray spectral evolution in an X-ray changing-look AGN NGC 1365 with variable column density
DOI: 10.1088/1674-4527/21/8/199 Bibcode: 2021RAA....21..199L

Liu, Hao; Yang, Jun; Wang, Ting-Gui +4 more

X-ray changing-look active galactic nuclei (CL AGNs) are a subpopulation of AGNs, whose line-of-sight column densities increase/decrease within several years. The physical mechanism for the variation of column density is unclear. We reduce the X-ray data from XMM-Newton and NuSTAR observations for a CL AGN NGC 1365 with strong variation of column …

2021 Research in Astronomy and Astrophysics
XMM-Newton 5
Detecting the intrinsic X-ray emission from the O-type donor star and the residual accretion in a supergiant fast X-ray transient in its faintest state
DOI: 10.1051/0004-6361/202141378 Bibcode: 2021A&A...654A.131S

Salvaterra, R.; Marelli, M.; Sidoli, L. +4 more

We report on the results of an XMM-Newton observation of the supergiant fast X-ray transient (SFXT) IGR J08408-4503 performed in June 2020. The source is composed of a compact object (likely a neutron star) orbiting around an O8.5Ib-II(f)p star, LM Vel. The X-ray light curve shows a very low level of emission, punctuated by a single, faint flare. …

2021 Astronomy and Astrophysics
Gaia XMM-Newton 5
Midsummer Atmospheric Changes in Saturn's Northern Hemisphere from the Hubble OPAL Program
DOI: 10.3847/PSJ/abe40f Bibcode: 2021PSJ.....2...47S

Wong, Michael H.; Hueso, Ricardo; Sánchez-Lavega, Agustín +1 more

Using the Hubble Space Telescope, Saturn was observed in 2018, 2019, and 2020, just after the northern hemisphere summer solstice. Analysis of multispectral imaging data reveals three years of cloud changes associated with a 70° N storm that began in 2018. Additionally, there is an increase in equatorial brightness and perhaps haze optical depth a…

2021 The Planetary Science Journal
eHST 5
Terahertz Water Masers. II. Further SOFIA/GREAT Detections Toward Circumstellar Outflows, and a Multitransition Analysis
DOI: 10.3847/1538-4357/abc628 Bibcode: 2021ApJ...907...42N

Wyrowski, Friedrich; Menten, Karl M.; Wiesemeyer, Helmut +8 more

Following up on our discovery of terahertz water masers, reported in 2017, we report two further detections of water maser emission at frequencies above 1 THz. Using the GREAT instrument on SOFIA, we have detected emission in the 1.296411 THz 827 - 734 transition of water toward two additional oxygen-rich evolved stars, omicr…

2021 The Astrophysical Journal
Gaia 5
Ground Vibrational State SiO Emission in the VLA BAaDE Survey
DOI: 10.3847/1538-3881/abd479 Bibcode: 2021AJ....161..111D

Rich, R. M.; Morris, M. R.; Claussen, M. J. +5 more

Using a subsample of the Bulge Asymmetries and Dynamical Evolution (BAaDE) survey of stellar SiO masers, we explore the prevalence and characteristics of 28SiO J = 1 - 0, v = 0 emission. We identify 90 detections of maser, thermal, or composite 28SiO J = 1 - 0, v = 0 emission out of approximately 13,000 candidate spectra from…

2021 The Astronomical Journal
Gaia 5
X-ray study of Abell 3365 with XMM-Newton
DOI: 10.1051/0004-6361/201937160 Bibcode: 2021A&A...646A..95U

Urdampilleta, I.; Simionescu, A.; Kaastra, J. S. +5 more

We present an X-ray spectral analysis using XMM-Newton/EPIC observations (∼100 ks) of the merging galaxy cluster Abell 3365 (z = 0.093). Previous radio observations suggested the presence of a peripheral elongated radio relic to the east and a smaller radio relic candidate to the west of the cluster center. We find evidence of temperature disconti…

2021 Astronomy and Astrophysics
XMM-Newton 5