Search Publications

An 8.56 keV Absorption Line in the Hyperluminous X-Ray Source in NGC 4045: Ultrafast Outflow or Cyclotron Line?
DOI: 10.3847/1538-4357/ac5e37 Bibcode: 2022ApJ...929..138B

Fürst, Felix; Middleton, Matthew J.; Walton, Dominic J. +5 more

We report on the discovery of an absorption line at $E={8.56}_{-0.11}^{+0.05}$ keV detected with a significance of >3.3σ in the NuSTAR and XMM-Newton spectra of a newly discovered hyperluminous X-ray source (L X > 1041 erg s-1) in the galaxy NGC 4045 at a distance of 32 Mpc. The source was first discovered se…

2022 The Astrophysical Journal
Gaia XMM-Newton 10
The Solar Internetwork. III. Unipolar versus Bipolar Flux Appearance
DOI: 10.3847/1538-4357/ac37be Bibcode: 2022ApJ...925..188G

Cheung, M. C. M.; Gošić, M.; Bellot Rubio, L. R. +3 more

Small-scale internetwork (IN) magnetic fields are considered to be the main building blocks of quiet Sun magnetism. For this reason, it is crucial to understand how they appear on the solar surface. Here, we employ a high-resolution, high-sensitivity, long-duration Hinode/NFI magnetogram sequence to analyze the appearance modes and spatiotemporal …

2022 The Astrophysical Journal
Hinode 10
Probing infrared excess connection with Li enhancement among red clump giants
DOI: 10.1093/mnras/stac224 Bibcode: 2022MNRAS.511.3741M

Reddy, Bacham E.; Muthumariappan, C.; Mallick, Anohita

We have performed a search among low-mass red giants for finding evidence for merger scenario for triggering He-flash and subsequent Li enhancement. We chose a sample of red giants from GALAH survey with well-measured Li abundances, and near- and mid-IR fluxes from 2MASS and WISE surveys, respectively. The sample contains 418 cool red clump giants…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 10
The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel
DOI: 10.1093/mnras/stac145 Bibcode: 2022MNRAS.511.1408G

Massardi, M.; Enia, A. F. M.; Negrello, M. +6 more

We investigate the radio/far-infrared (FIR) correlation for a sample of 28 bright high-redshift (1 ≲ z ≲ 4) star-forming galaxies selected in the FIR from the Herschel-ATLAS fields as candidates to be strongly gravitationally lensed. The radio information comes either from high sensitivity dedicated Australia Telescope Compact Array observations a…

2022 Monthly Notices of the Royal Astronomical Society
eHST 10
Search for primordial black hole dark matter with x-ray spectroscopic and imaging satellite experiments and prospects for future satellite missions
DOI: 10.1103/PhysRevD.106.123020 Bibcode: 2022PhRvD.106l3020M

Santangelo, Andrea; Malyshev, Denys; Moulin, Emmanuel

Ultralight primordial black holes (PBHs) in the mass range of 1016- 1022 g are allowed by current observations to constitute a significant fraction, if not all, of the dark matter in the Universe. In this work, we present limits on ultralight, nonrotating PBHs which arise from the nondetection of the Hawking radiation signals…

2022 Physical Review D
INTEGRAL XMM-Newton 10
Bayesian Inference in Single-line Spectroscopic Binaries with a Visual Orbit
DOI: 10.3847/1538-3881/ac5ab4 Bibcode: 2022AJ....163..220V

Mendez, Rene A.; Clavería, Rubén M.; Orchard, Marcos E. +2 more

We present a Bayesian inference methodology for the estimation of orbital parameters on single-line spectroscopic binaries with astrometric data, based on the No-U-Turn sampler Markov chain Monte Carlo algorithm. Our approach is designed to provide a precise and efficient estimation of the joint posterior distribution of the orbital parameters in …

2022 The Astronomical Journal
Gaia 10
Properties and applications of a predicted population of runaway He-sdO/B stars ejected from single degenerate He-donor SNe
DOI: 10.1051/0004-6361/202142864 Bibcode: 2022A&A...663A..91N

Geier, S.; Justham, S.; Neunteufel, P. +4 more

Context. Thermonuclear supernovae (SNe), a subset of which are the highly important SNe of Type Ia and Iax, are relatively poorly understood phenomena. One of the more promising scenarios leading up to the creation of a thermonuclear SN involves accretion of helium-rich material from a binary companion. Following the SN, the binary companion is th…

2022 Astronomy and Astrophysics
Gaia 10
Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
DOI: 10.3847/1538-4357/ac7051 Bibcode: 2022ApJ...933...30T

Matharu, Jasleen; Muzzin, Adam; van der Wel, Arjen +9 more

One of the challenges in understanding the quenching processes for galaxies is connecting progenitor star-forming populations to their descendant quiescent populations over cosmic time. Here we attempt a novel approach to this challenge by assuming that the underlying stellar mass distribution of galaxies is not significantly altered during enviro…

2022 The Astrophysical Journal
eHST 10
Quasar and galaxy classification using Gaia EDR3 and CatWise2020
DOI: 10.1051/0004-6361/202244859 Bibcode: 2022A&A...668A..99H

Bailer-Jones, Coryn A. L.; Hughes, Arvind C. N.; Jamal, Sara

In this work, we assess the combined use of Gaia photometry and astrometry with infrared data from CatWISE in improving the identification of extragalactic sources compared to the classification obtained using Gaia data. Here we perform a comprehensive study in which we assess different input feature configurations and prior functions to identify …

2022 Astronomy and Astrophysics
Gaia 10
IM Normae: The Death Spiral of a Cataclysmic Variable?
DOI: 10.3847/1538-4357/abec87 Bibcode: 2022ApJ...924...27P

Myers, Gordon; Monard, Berto; Dvorak, Shawn +18 more

We present a study of the orbital light curves of the recurrent nova IM Normae since its 2002 outburst. The broad "eclipses" recur with a 2.46 hr period, which increases on a timescale of 1.28(16) × 106 yr. Under the assumption of conservative mass transfer, this suggests a rate near 10-7 M yr-1, and t…

2022 The Astrophysical Journal
Gaia 10