Search Publications

Orbital and atmospheric parameters of two wide O-type subdwarf binaries: BD−11o162 and Feige 80
DOI: 10.1051/0004-6361/202141220 Bibcode: 2022A&A...658A.122M

Németh, Péter; Tkachenko, Andrew; van Winckel, Hans +4 more

Context. There are 23 long-period binary systems discovered to date that contain a B-type hot subdwarf whose orbital parameters have been fully solved. They evolve into O-type subdwarfs (sdO) once the helium burning transitions from the core to the He shell. Their study will help constraint parameters on the formation and evolution of these binari…

2022 Astronomy and Astrophysics
Gaia 6
An intermediate polar candidate toward the Galactic plane
DOI: 10.1051/0004-6361/202244264 Bibcode: 2022A&A...666A.150M

Campana, S.; Haberl, F.; Ponti, G. +5 more

Context. For the past decade, it has been suggested that intermediate polars (IPs), a subclass of magnetic cataclysmic variables (CVs), are one of the main contributors to the hard diffuse X-ray emission from the Galactic center (GC) and Galactic ridge.
Aims: In our ongoing XMM-Newton survey of the central region of the Galactic disk (20° ×2°…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 6
Convective storms in closed cyclones in Jupiter: (II) numerical modeling
DOI: 10.1016/j.icarus.2022.115169 Bibcode: 2022Icar..38615169I

Hueso, Ricardo; Sánchez-Lavega, Agustín; Legarreta, Jon +1 more

On May 31, 2020 a convective storm appeared in one small cyclone in the South Temperate Belt (STB) of Jupiter. The storm, nicknamed as Clyde's Spot, had an explosive start and quickly diminished in activity in a few days. However, it left a highly turbulent cyclone as a remnant that evolved to become a turbulent segment of the STB in a time-scale …

2022 Icarus
eHST 6
Analytic modeling of recurrent Forbush decreases caused by corotating interaction regions
DOI: 10.1051/0004-6361/202140846 Bibcode: 2022A&A...658A.186V

Vršnak, B.; Dumbović, M.; Heber, B. +1 more

Context. On scales of days, the galactic cosmic ray (GCR) flux is affected by coronal mass ejections and corotating interaction regions (CIRs), causing so-called Forbush decreases and recurrent Forbush decreases (RFDs), respectively.
Aims: We explain the properties and behavior of RFDs recorded at about 1 au that are caused by CIRs generated …

2022 Astronomy and Astrophysics
SOHO 6
On the Characterization of GJ 504: A Magnetically Active Planet-host Star Observed by the Transiting Exoplanet Survey Satellite (TESS)
DOI: 10.3847/1538-4357/ac8f44 Bibcode: 2022ApJ...940...93D

Stassun, Keivan G.; García, Rafael A.; Corsaro, Enrico +11 more

We present the results of the analysis of the photometric data collected in long- and short-cadence mode by the Transiting Exoplanet Survey Satellite for GJ 504, a well-studied planet-hosting solar-like star, whose fundamental parameters have been largely debated during the last decade. Several attempts have been made by the present authors to iso…

2022 The Astrophysical Journal
Gaia 6
Numerical simulations of radar echoes rule out basal CO2 ice deposits at Ultimi Scopuli, Mars
DOI: 10.1016/j.icarus.2022.115163 Bibcode: 2022Icar..38615163O

Orosei, Roberto; Cartacci, Marco; Cicchetti, Andrea +10 more

The principal objective of the radar sounder MARSIS experiment is to look for ice and water in the Martian subsurface. One particular focus of investigations, since 2005, has been the search for basal liquid water in the south polar layered deposits (SPLD). Anomalously strong basal echoes detected from four distinct areas at the base of the deposi…

2022 Icarus
MEx 6
Using Multiple Emission Line Ratios to Constrain the Slope of the Dust Attenuation Law
DOI: 10.3847/1538-4357/ac5459 Bibcode: 2022ApJ...928...71P

Papovich, Casey; Cleri, Nikko J.; Trump, Jonathan R. +2 more

We explore the possibility and practical limitations of using a three-line approach to measure both the slope and normalization of the dust attenuation law in individual galaxies. To do this, we focus on a sample of 11 galaxies with existing ground-based Balmer Hα and Hβ measurements from slit spectra, plus space-based grism constraints on Paschen…

2022 The Astrophysical Journal
eHST 6
The Missing Metal Problem in Galaxy Clusters: Characterizing the Early Enrichment Population
DOI: 10.3847/1538-4357/ac4dfb Bibcode: 2022ApJ...927..104B

Bregman, Joel N.; Blackwell, Anne E.; Snowden, Steven L.

Rich and poor galaxy clusters have the same measured halo metallicity, 0.35-0.4 Z , even though they are an order of magnitude apart in stellar fraction, M */M gas. The measured intracluster medium (ICM) metallicity in high-mass clusters cannot be explained by the visible stellar population as stars typically make…

2022 The Astrophysical Journal
XMM-Newton 6
HORuS transmission spectroscopy and revised planetary parameters of KELT-7 b
DOI: 10.1093/mnras/stac1759 Bibcode: 2022MNRAS.515.1247T

Rebolo, R.; del Burgo, C.; Montes, D. +7 more

We report on the high-resolution spectroscopic observations of two planetary transits of the hot Jupiter KELT-7b (Mp = 1.28 ± 0.17MJup, Teq = 2028 K) observed with the High Optical Resolution Spectrograph (HORuS) mounted on the 10.4-m Gran Telescopio Canarias (GTC). A new set of stellar parameters are obtained for …

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 6
Galaxy Rotation Parameters from OB2 Stars with Proper Motions and Parallaxes from the Gaia EDR3 Catalog
DOI: 10.1134/S1063772922040011 Bibcode: 2022ARep...66..269B

Bobylev, V. V.; Bajkova, A. T.

We have analyzed the kinematics of OB2 stars with proper motions and parallaxes selected by Xu et al. from the Gaia EDR3 catalog. The relative parallax errors for all the stars in this sample do not exceed 10%. Based on a sample of 9750 stars, the group velocity components ${{(U,V,W)}_{ \odot }} = $ (7.21, 7.46, 8.52) ± (0.13, 0.20, 0.10) km/s wer…

2022 Astronomy Reports
Gaia 6