Search Publications

CO2-driven surface changes in the Hapi region on Comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stac2560 Bibcode: 2022MNRAS.516.6009D

Da Deppo, Vania; Lellouch, Emmanuel; Buratti, Bonnie J. +24 more

Between 2014 December 31 and 2015 March 17, the OSIRIS cameras on Rosetta documented the growth of a $140\, \mathrm{\hbox{-}m}$ wide and $0.5\, \mathrm{\hbox{-}m}$ deep depression in the Hapi region on Comet 67P/Churyumov-Gerasimenko. This shallow pit is one of several that later formed elsewhere on the comet, all in smooth terrain that primarily …

2022 Monthly Notices of the Royal Astronomical Society
Rosetta 10
Investigation of the negative ionospheric response of the 8 September 2017 geomagnetic storm over the European sector
DOI: 10.1016/j.asr.2022.05.035 Bibcode: 2022AdSpR..70.1104O

Oikonomou, Christina; Haralambous, Haris; Paul, Ashik +4 more

In this study, we investigate the negative ionospheric response over the European sector during two storms that took place on 8 September 2017, primarily, by exploiting observations over ten European locations. The spatial and temporal variations of TEC, foF2 and hmF2 ionospheric characteristics are examined with the aim to explain the physical me…

2022 Advances in Space Research
SOHO 10
Gaia search for stellar companions of TESS Objects of Interest III
DOI: 10.1002/asna.20224017 Bibcode: 2022AN....34324017M

Mugrauer, Markus; Michel, Kai-Uwe; Zander, Jule

The latest results from our ongoing multiplicity study of (Community) TESS Objects of Interest are presented, using astro- and photometric data from the ESA-Gaia mission, to detect stellar companions of these stars and characterize their properties. A total of 124 binary and 7 hierarchical triple star systems were detected among 2175 targets, whos…

2022 Astronomische Nachrichten
Gaia 10
White-dwarf asteroseismology with the TESS space telescope
DOI: 10.48550/arXiv.2203.03769 Bibcode: 2022BAAA...63...48C

Córsico, A. H.

As white-dwarf (WD) stars cool, they go through one or more stages of g(gravity)-mode pulsational instability, becoming multiperiodic variable stars. Stars passing through these instability domains allow astronomers to study their interiors through asteroseismological techniques, as if they could ``look'' at their interiors by analyzing the spectr…

2022 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 10
First detection of AlF line emission towards M-type AGB stars
DOI: 10.1051/0004-6361/202141704 Bibcode: 2022A&A...663A..54S

Fonfría, J. P.; Velilla-Prieto, L.; Wedemeyer, S. +3 more

The nucleosynthesis production of fluorine (F) is still a matter of debate. Asymptotic giant branch (AGB) stars are one of the main candidates for F production. However, their contribution to the total F budget is not fully known due to the lack of observations. In this paper, we report the detection of aluminium monofluoride (AlF) line emission, …

2022 Astronomy and Astrophysics
ISO 10
Fundamental Properties of Late-Type Stars in Eclipsing Binaries
DOI: 10.3390/galaxies10050098 Bibcode: 2022Galax..10...98M

Ribas, Ignasi; Giménez, Álvaro; Morales, Juan Carlos +1 more

Evidence from the analysis of eclipsing binary systems revealed that late-type stars are larger and cooler than predicted by models, and that this is probably caused by stellar magnetic activity. In this work, we revisit this problem taking into account the advancements in the last decade. We provide and updated a list of 32 eclipsing binary or mu…

2022 Galaxies
Gaia 10
Flaring-associated Complex Dynamics in Two M Dwarfs Revealed by Fast, Time-resolved Spectroscopy
DOI: 10.3847/1538-4357/ac7a35 Bibcode: 2022ApJ...934...98W

Wang, J.; Li, H. L.; Xin, L. P. +11 more

Habitability of an exoplanet is believed to be profoundly affected by activities of the host stars, although the related coronal mass ejections (CMEs) are still rarely detected in solar-like and late-type stars. We here report an observational study on the flares of two M dwarfs triggered by the high-cadence survey performed by the Ground-based Wi…

2022 The Astrophysical Journal
Gaia 10
The Paschen Jump as a Diagnostic of the Diffuse Nebular Continuum Emission in Active Galactic Nuclei
DOI: 10.3847/1538-4357/ac4bc6 Bibcode: 2022ApJ...927...60G

Ho, Luis C.; Brandt, William N.; Barth, Aaron J. +17 more

Photoionization modeling of active galactic nuclei (AGN) predicts that diffuse continuum (DC) emission from the broad-line region makes a substantial contribution to the total continuum emission from ultraviolet through near-infrared wavelengths. Evidence for this DC component is present in the strong Balmer jump feature in AGN spectra, and possib…

2022 The Astrophysical Journal
eHST 10
A Submillimeter Survey of Faint Galaxies behind 10 Strong Lensing Clusters
DOI: 10.3847/1538-4357/ac91d2 Bibcode: 2022ApJ...939....5C

Bauer, F. E.; Barger, A. J.; Cowie, L. L. +5 more

We present deep SCUBA-2 450 µm and 850 µm imaging of 10 strong lensing clusters. We provide a >4σ SCUBA-2 850 µm catalog of the 404 sources lying within a radius of $4\buildrel{\,\prime}\over{.} 5$ from the cluster centers. We also provide catalogs of the >4.5σ Atacama Large Millimeter/submillimeter Array (ALMA) 850 µ…

2022 The Astrophysical Journal
Herschel eHST 10
Viewing Angle Observations and Effects of Evolution with Redshift, Black Hole Mass, and Eddington Ratio in Quasar-based Cosmology
DOI: 10.3847/1538-4357/ac3f36 Bibcode: 2022ApJ...925..215P

Pollo, Agnieszka; Czerny, Bożena; Prince, Raj +2 more

This study is focused on the observational measurement of the viewing angle of individual quasars by modeling the broadband quasar spectrum ranging from the IR to soft X-ray band. Sources are selected from various published catalogs, and their broadband quasi-simultaneous spectral data points were collected and used for modeling. We started with a…

2022 The Astrophysical Journal
XMM-Newton 10