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The Heliosphere and Local Interstellar Medium from Neutral Atom Observations at Energies Below 10 keV
DOI: 10.1007/s11214-022-00901-7 Bibcode: 2022SSRv..218...31G

Schwadron, Nathan A.; Izmodenov, Vladislav V.; Kucharek, Harald +8 more

As the heliosphere moves through the surrounding interstellar medium, a fraction of the interstellar neutral helium, hydrogen, and heavier species crossing the heliopause make it to the inner heliosphere as neutral atoms with energies ranging from few eV to several hundred eV. In addition, energetic neutral hydrogen atoms originating from solar wi…

2022 Space Science Reviews
SOHO Ulysses 18
Pulsating B stars in the Scorpius-Centaurus Association with TESS
DOI: 10.1093/mnras/stac1816 Bibcode: 2022MNRAS.515..828S

Bedding, Timothy R.; White, Timothy R.; Saio, Hideyuki +1 more

We study 119 B stars located in the Scorpius-Centaurus Association using data from NASA's TESS Mission. We see pulsations in 81 stars (68 per cent) across the full range of effective temperatures. In particular, we confirm previous reports of low-frequency pulsations in stars whose temperatures fall between the instability strips of SPB stars (slo…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18
An extended stellar halo discovered in the Fornax dwarf spheroidal using Gaia EDR3
DOI: 10.1093/mnras/stac644 Bibcode: 2022MNRAS.512.4171Y

Hammer, François; Pawlowski, Marcel S.; Yang, Yanbin +1 more

We have studied the extent of the Red Giant Branch stellar population in the Fornax dwarf spheroidal galaxy using the spatially extended and homogeneous data set from Gaia EDR3. Our pre-selection of stars belonging to Fornax is based on their proper motions, parallaxes, and colour-magnitude diagram. The latter criteria provide a Fornax star sample…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18
Application of a Steady-state Accretion Disk Model to Spectrophotometry and High-resolution Spectra of Two Recent FU Ori Outbursts
DOI: 10.3847/1538-4357/ac496b Bibcode: 2022ApJ...927..144R

Rodriguez, Antonio C.; Hillenbrand, Lynne A.

We apply a conventional accretion disk model to the FU Ori-type objects HBC 722 and Gaia 17bpi. Our base model is a steady-state, thin Keplerian disk featuring a modified Shakura-Sunyaev temperature profile, with each annulus radiating as an area-weighted spectrum given by a NextGen atmosphere at the appropriate temperature. We explore departures …

2022 The Astrophysical Journal
Gaia 18
High-density disc reflection spectroscopy of low-mass active galactic nuclei
DOI: 10.1093/mnras/stac990 Bibcode: 2022MNRAS.513.4361M

Fabian, A. C.; Pinto, C.; Gandhi, P. +13 more

The standard alpha-disc model predicts an anticorrelation between the density of the inner accretion disc and the black hole mass times square of the accretion rate, as seen in higher mass (MBH > 106 M) active galactic nuclei (AGNs). In this work, we test the predictions of the alpha-disc model and study the pr…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
The Fundamental Planes of black hole activity for radio-loud and radio-quiet quasars
DOI: 10.1093/mnras/stac1153 Bibcode: 2022MNRAS.513.4673B

Snios, Bradford; Siemiginowska, Aneta; Schwartz, Daniel A. +2 more

We examine the Fundamental Plane of black hole activity for correlations with redshift and radio loudness in both radio-loud and radio-quiet quasar populations. Sources are compiled from archival data of both radio-loud and radio-quiet quasars over redshifts 0.1 < z < 5.0 to produce a sample of 353 sources with known X-ray, radio, and black …

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
The Galactic Nova Rate: Estimates from the ASAS-SN and Gaia Surveys
DOI: 10.3847/1538-4357/ac8d5e Bibcode: 2022ApJ...937...64K

Mukai, K.; Kochanek, C. S.; Hodgkin, S. T. +13 more

We present the first estimate of the Galactic nova rate based on optical transient surveys covering the entire sky. Using data from the All-Sky Automated Survey for Supernovae (ASAS-SN) and Gaia-the only two all-sky surveys to report classical nova candidates-we find 39 confirmed Galactic novae and 7 additional unconfirmed candidates discovered fr…

2022 The Astrophysical Journal
Gaia 18
Interrogating Solar Flare Loop Models with IRIS Observations 1: Overview of the Models, and Mass flows
DOI: 10.3389/fspas.2022.1060856 Bibcode: 2022FrASS...960856K

Kerr, Graham S.

Solar and stellar flares are transient yet dramatic events in the atmospheres of the Sun or stars, during which vast amounts of magnetic energy is liberated. This energy is subsequently transported through the solar atmosphere or into the heliosphere, and together with coronal mass ejections flares comprise a fundamental component of space weather…

2022 Frontiers in Astronomy and Space Sciences
IRIS 18
The CARMENES search for exoplanets around M dwarfs. Two Saturn-mass planets orbiting active stars
DOI: 10.1051/0004-6361/202142915 Bibcode: 2022A&A...663A..48Q

Amado, P. J.; Caballero, J. A.; Pallé, E. +26 more

The CARMENES radial-velocity survey is currently searching for planets in a sample of 387 M dwarfs. Here we report on two Saturn-mass planets orbiting TYC 2187-512-1 (M* = 0.50 M) and TZ Ari (M* = 0.15 M), respectively. We obtained supplementary photometric time series, which we use along with spectros…

2022 Astronomy and Astrophysics
Gaia 18
A Young, Low-density Stellar Stream in the Milky Way Disk: Theia 456
DOI: 10.3847/1538-3881/ac6952 Bibcode: 2022AJ....163..275A

Kounkel, Marina; Covey, Kevin R.; Agüeros, Marcel A. +4 more

Our view of the variety of stellar structures pervading the local Milky Way has been transformed by the application of clustering algorithms to the Gaia catalog. In particular, several stellar streams have been recently discovered that are comprised of hundreds to thousands of stars and span several hundred parsecs. We analyze one such structure, …

2022 The Astronomical Journal
Gaia 18