Search Publications

The Close AGN Reference Survey (CARS). Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044
DOI: 10.1051/0004-6361/202243697 Bibcode: 2022A&A...663A.104W

Jahnke, K.; Gaspari, M.; Combes, F. +11 more

Context. The host galaxy conditions for rapid supermassive black hole growth are poorly understood. Narrow-line Seyfert 1 (NLS1) galaxies often exhibit high accretion rates and are hypothesized to be prototypes of active galactic nuclei (AGN) at an early stage of their evolution.
Aims: We present adaptive optics (AO) assisted VLT MUSE NFM obs…

2022 Astronomy and Astrophysics
eHST 12
Uniform Recalibration of Common Spectrophotometry Standard Stars onto the CALSPEC System Using the SuperNova Integral Field Spectrograph
DOI: 10.3847/1538-4365/ac7b7f Bibcode: 2022ApJS..263....1R

Aldering, G.; Kim, A. G.; Kowalski, M. +35 more

We calibrate spectrophotometric optical spectra of 32 stars commonly used as standard stars, referenced to 14 stars already on the Hubble Space Telescope-based CALSPEC flux system. Observations of CALSPEC and non-CALSPEC stars were obtained with the SuperNova Integral Field Spectrograph over the wavelength range 3300-9400 Å as calibration for the …

2022 The Astrophysical Journal Supplement Series
Gaia 12
An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
DOI: 10.3847/1538-4357/ac626c Bibcode: 2022ApJ...930...81J

Smith, Nathan; Strader, Jay; Sand, David J. +6 more

We present the discovery of an exceptional dimming event in a cool supergiant star in the Local Volume spiral M51. The star, dubbed M51-DS1, was found as part of a Hubble Space Telescope (HST) search for failed supernovae (SNe). The supergiant, which is plausibly associated with a very young (≲6 Myr) stellar population, showed clear variability (a…

2022 The Astrophysical Journal
eHST 12
A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers during the Third Gravitational-wave Observing Run
DOI: 10.3847/1538-4357/ac4d34 Bibcode: 2022ApJ...927...50R

Fong, W.; Sand, D. J.; Rastinejad, J. C. +9 more

We present a comprehensive analysis of 653 optical candidate counterparts reported during the third gravitational-wave (GW) observing run. Our sample concentrates on candidates from the 15 events (published in GWTC-2, GWTC-3, or not retracted on GraceDB) that had a >1% chance of including a neutron star in order to assess their viability as tru…

2022 The Astrophysical Journal
Gaia 12
SN 1987A: Tracing the flux decline and spectral evolution through a comparison of SRG/eROSITA and XMM-Newton observations
DOI: 10.1051/0004-6361/202141104 Bibcode: 2022A&A...661A..30M

Haberl, F.; Freyberg, M. J.; Maggi, P. +3 more

Context. SN 1987A is the supernova closest to us observed in the past four centuries. It provides the unique opportunity of witnessing the birth and evolution of a supernova remnant. Monitoring the source in X-rays provides insights into the physics of the shock, the X-ray emitting plasma, and the interaction of the shock with the structures in th…

2022 Astronomy and Astrophysics
XMM-Newton 12
How to search for mirror stars with Gaia
DOI: 10.1007/JHEP07(2022)059 Bibcode: 2022JHEP...07..059H

Matzner, Christopher D.; Curtin, David; Howe, Aaron +1 more

We show for the first time how to conduct a direct search for dark matter using Gaia observations. Its public astrometric data may contain the signals of mirror stars, exotic compact objects made of atomic dark matter with a tiny kinetic mixing between the dark and SM photon. Mirror stars capture small amounts of interstellar material in their cor…

2022 Journal of High Energy Physics
Gaia 12
Constraining the overcontact phase in massive binary evolution. II. Period stability of known O+O overcontact systems
DOI: 10.1051/0004-6361/202244148 Bibcode: 2022A&A...666A..18A

Mahy, Laurent; Abdul-Masih, Michael; Marchant, Pablo +2 more

Context. Given that mergers are often invoked to explain many exotic phenomena in massive star evolution, understanding the evolutionary phase directly preceding a merger, the overcontact phase, is of crucial importance. Despite this, large uncertainties exist in our understanding of the evolution of massive overcontact binaries.
Aims: We aim…

2022 Astronomy and Astrophysics
INTEGRAL 12
Coronal Mass Ejections and Type II Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani
DOI: 10.3847/1538-4357/ac35de Bibcode: 2022ApJ...924..115O

Ó Fionnagáin, Dúalta; Kavanagh, Robert D.; Vidotto, Aline A. +5 more

We simulate possible stellar coronal mass ejection (CME) scenarios over the magnetic cycle of ϵ Eridani (18 Eridani; HD 22049). We use three separate epochs from 2008, 2011, and 2013, and estimate the radio emission frequencies associated with these events. These stellar eruptions have proven to be elusive, although a promising approach to detect …

2022 The Astrophysical Journal
Gaia 12
KIC 7955301: A hierarchical triple system with eclipse timing variations and an oscillating red giant
DOI: 10.1051/0004-6361/202244373 Bibcode: 2022A&A...668A.173G

Borkovits, Tamás; Miglio, Andrea; Appourchaux, Thierry +13 more

KIC 7955301 is a hierarchical triple system with clear eclipse timing and depth variations that was discovered by the Kepler satellite during its original mission. It is composed of a non-eclipsing primary star at the bottom of the red giant branch (RGB) on a 209-day orbit with a K/G-type main-sequence (MS) inner eclipsing binary (EB), orbiting in…

2022 Astronomy and Astrophysics
Gaia 12
Radio monitoring of transient Be/X-ray binaries and the inflow-outflow coupling of strongly magnetized accreting neutron stars
DOI: 10.1093/mnras/stac2518 Bibcode: 2022MNRAS.516.4844V

Degenaar, N.; Wijnands, R.; Miller-Jones, J. C. A. +5 more

Strongly magnetized (B ≥ 1012 G) accreting neutron stars (NSs) are prime targets for studying the launching of jets by objects with a solid surface; while classical jet-launching models predict that such NSs cannot launch jets, recent observations and models argue otherwise. Transient Be/X-ray binaries (BeXRBs) are critical laboratories…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 12