Search Publications

The Evolution of Plasma Composition during a Solar Flare
DOI: 10.3847/1538-4357/abe85a Bibcode: 2021ApJ...911...86T

Long, David M.; Brooks, David H.; Baker, Deborah +4 more

We analyze the coronal elemental abundances during a small flare using Hinode/EIS observations. Compared to the preflare elemental abundances, we observed a strong increase in coronal abundance of Ca XIV 193.84 Å, an emission line with low first ionization potential (FIP < 10 eV), as quantified by the ratio Ca/Ar during the flare. This is in co…

2021 The Astrophysical Journal
Hinode 20
The substructure of the Perseus star-forming region: a survey with Gaia DR2
DOI: 10.1093/mnras/stab352 Bibcode: 2021MNRAS.503.3232P

Scholz, Aleks; Teixeira, Paula S.; Pavlidou, Tatiana

We use photometric and kinematic data from Gaia DR2 to explore the structure of the star-forming region associated with the molecular cloud of Perseus. Apart from the two well-known clusters, IC 348 and NGC 1333, we present five new clustered groups of young stars, which contain between 30 and 300 members, named Autochthe, Alcaeus, Heleus, Electry…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 20
First Detection of Orbital Motion for HD 106906 b: A Wide-separation Exoplanet on a Planet Nine-like Orbit
DOI: 10.3847/1538-3881/abc012 Bibcode: 2021AJ....161...22N

Kalas, Paul; De Rosa, Robert J.; Nguyen, Meiji M.

HD 106906 is a 15 Myr old short-period (49 days) spectroscopic binary that hosts a wide-separation (737 au) planetary-mass ( $\sim 11\,{M}_{\mathrm{Jup}}$ ) common proper motion companion, HD 106906 b. Additionally, a circumbinary debris disk is resolved at optical and near-infrared wavelengths that exhibits a significant asymmetry at wide separat…

2021 The Astronomical Journal
Gaia eHST 20
The 6.2 µm PAH Feature and the Role of Nitrogen: Revisited
DOI: 10.3847/1538-4357/ac28fc Bibcode: 2021ApJ...923..202R

Boersma, C.; Peeters, E.; Ricca, A.

This study revisits the role that nitrogen inclusion in polycyclic aromatic hydrocarbons (PAHs; those with nitrogen inclusion, PANHs) plays in their infrared (IR) spectral properties. We present spectra of pure PAHs, PANHs, and protonated PANHs, computed using density functional theory and basis sets that treat polarization. We investigate trends …

2021 The Astrophysical Journal
ISO eHST 20
TOI-1431b/MASCARA-5b: A Highly Irradiated Ultrahot Jupiter Orbiting One of the Hottest and Brightest Known Exoplanet Host Stars
DOI: 10.3847/1538-3881/ac224e Bibcode: 2021AJ....162..292A

Latham, David W.; Stassun, Keivan G.; Wittenmyer, Robert A. +70 more

We present the discovery of a highly irradiated and moderately inflated ultrahot Jupiter, TOI-1431b/MASCARA-5 b (HD 201033b), first detected by NASA's Transiting Exoplanet Survey Satellite mission (TESS) and the Multi-site All-Sky Camera (MASCARA). The signal was established to be of planetary origin through radial velocity measurements obtained u…

2021 The Astronomical Journal
Gaia 20
The PAU Survey: narrow-band photometric redshifts using Gaussian processes
DOI: 10.1093/mnras/stab711 Bibcode: 2021MNRAS.503.4118S

Alarcon, Alex; Carretero, Jorge; Castander, Francisco J. +16 more

We study the performance of the hybrid template machine learning photometric redshift (photo-z) algorithm DELIGHT, which uses Gaussian processes, on a subset of the early data release of the Physics of the Accelerating Universe Survey (PAUS). We calibrate the fluxes of the 40 PAUS narrow bands with six broad-band fluxes (uBVriz) in the Cosmic Evol…

2021 Monthly Notices of the Royal Astronomical Society
eHST 20
Broadband X-ray spectral variability of the pulsing ULX NGC 1313 X-2
DOI: 10.1051/0004-6361/202140884 Bibcode: 2021A&A...652A.118R

Cusumano, G.; Fabian, A. C.; Pinto, C. +12 more

Context. It is thought that ultraluminous X-ray sources (ULXs) are mainly powered by super-Eddington accreting neutron stars or black holes as shown by the recent discovery of X-ray pulsations and relativistic winds.
Aims: This work presents a follow-up study of the spectral evolution over two decades of the pulsing ULX NGC 1313 X-2 in order …

2021 Astronomy and Astrophysics
XMM-Newton 20
A Catalog of Host Galaxies for WISE-selected AGN: Connecting Host Properties with Nuclear Activity and Identifying Contaminants
DOI: 10.3847/1538-4357/ac1352 Bibcode: 2021ApJ...922..179B

Stern, Daniel; Comerford, Julia M.; Barrows, R. Scott +1 more

We present a catalog of physical properties for galaxies hosting active galactic nuclei (AGN) detected by the Wide-field Infrared Survey Explorer (WISE). By fitting broadband spectral energy distributions of sources in the WISE AGN Catalog with empirical galaxy and AGN templates, we derive photometric redshifts, AGN bolometric luminosities, measur…

2021 The Astrophysical Journal
Gaia Herschel 20
Exploring the radial evolution of interplanetary coronal mass ejections using EUHFORIA
DOI: 10.1051/0004-6361/202040226 Bibcode: 2021A&A...649A..69S

Zhukov, A. N.; Rodriguez, L.; Poedts, S. +2 more

Context. Coronal mass ejections (CMEs) are large-scale eruptions coming from the Sun and transiting into interplanetary space. While it is widely known that they are major drivers of space weather, further knowledge of CME properties in the inner heliosphere is limited by the scarcity of observations at heliocentric distances other than 1 au. In a…

2021 Astronomy and Astrophysics
SOHO 20
Measuring the Magnetic Origins of Solar Flares, Coronal Mass Ejections, and Space Weather
DOI: 10.3847/1538-4357/ac081f Bibcode: 2021ApJ...917...27J

Rempel, Matthias; de Toma, Giuliana; Ezzeddine, Rana +12 more

We take a broad look at the problem of identifying the magnetic solar causes of space weather. With the lackluster performance of extrapolations based upon magnetic field measurements in the photosphere, we identify a region in the near-UV (NUV) part of the spectrum as optimal for studying the development of magnetic free energy over active region…

2021 The Astrophysical Journal
eHST 20