Search Publications

Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters: Limits from supermassive black hole x-ray data
DOI: 10.1103/PhysRevD.104.024058 Bibcode: 2021PhRvD.104b4058A

Tripathi, Ashutosh; Abdikamalov, Askar B.; Ayzenberg, Dimitry +2 more

X-ray reflection spectroscopy is a powerful technique for probing the nature of gravity around black holes in the so-called strong-field regime. One popular approach is to look at theory-agnostic deviations away from the Kerr solution, which is the only astrophysically relevant black hole solution within classical general relativity, in order to v…

2021 Physical Review D
XMM-Newton 12
Internal Structure of the 2019 April 2 CME
DOI: 10.3847/1538-4357/ac2aab Bibcode: 2021ApJ...922..234W

Vourlidas, Angelos; Wood, Brian E.; Braga, Carlos R.

We present the first analysis of internal coronal mass ejection (CME) structure observed very close to the Sun by the Wide-field Imager for Solar PRobe (WISPR) instrument on board the Parker Solar Probe (PSP). The transient studied here is a CME observed during PSP's second perihelion passage on 2019 April 2, when PSP was only 40 R fr…

2021 The Astrophysical Journal
SOHO 12
Understanding X-ray and optical selection of galaxy clusters: a comparison of the XXL and CAMIRA cluster catalogues obtained in the common XXL-HSC SSP area
DOI: 10.1093/mnras/stab873 Bibcode: 2021MNRAS.503.5624W

Okabe, N.; Chiappetti, L.; Altieri, B. +31 more

Large samples of galaxy clusters provide knowledge of both astrophysics in the most massive virialized environments and the properties of the cosmological model that defines our Universe. However, an important issue that affects the interpretation of galaxy cluster samples is the role played by the selection waveband and the potential for this to …

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
DOI: 10.3847/1538-4357/abf142 Bibcode: 2021ApJ...912..119R

Roederer, Ian U.; Lawler, James E.

We report the detection of an Al II line at 2669.155 Å in 11 metal-poor stars, using ultraviolet spectra obtained with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. We derive Al abundances from this line using a standard abundance analysis, assuming local thermodynamic equilibrium (LTE). The mean [Al/Fe] ratio is -0…

2021 The Astrophysical Journal
eHST 12
Multiwavelength Evidence for a New Flare-mode Transitional Millisecond Pulsar
DOI: 10.3847/1538-4357/ac0b47 Bibcode: 2021ApJ...917...69S

Strader, Jay; Bahramian, Arash; Chomiuk, Laura +7 more

We report the discovery of a new low-mass X-ray binary near the center of the unassociated Fermi GeV γ-ray source 4FGL J0540.0-7552. The source shows the persistent presence of an optical accretion disk and exhibits extreme X-ray and optical variability. It also has an X-ray spectrum well-fit by a hard power law with Γ = 1.8 and a high ratio of X-…

2021 The Astrophysical Journal
Gaia XMM-Newton 12
Long Term Evolution of Surface Features on the Red Supergiant AZ Cyg
DOI: 10.3847/1538-4357/ac0c7e Bibcode: 2021ApJ...919..124N

Gies, Douglas R.; Monnier, John D.; Schaefer, Gail H. +23 more

We present H-band interferometric observations of the red supergiant (RSG) AZ Cyg that were made with the Michigan Infra-Red Combiner (MIRC) at the six-telescope Center for High Angular Resolution Astronomy (CHARA) Array. The observations span 5 yr (2011-2016), which offers insight into the short and long-term evolution of surface features on RSGs…

2021 The Astrophysical Journal
Gaia 12
A fully-spectroscopic triple-source-plane lens: the Jackpot completed
DOI: 10.1093/mnras/stab1399 Bibcode: 2021MNRAS.505.2136S

Collett, Thomas E.; Smith, Russell J.

We present a spectroscopic determination of the redshift of the second source in the Jackpot gravitational lens system J0946 + 1006, for which only a photometric estimate of zphot = 2.41$^{+0.04}_{-0.21}$ has previously been available. By visually inspecting an archival Very Large Telescope (VLT) X-Shooter observation, we located a sing…

2021 Monthly Notices of the Royal Astronomical Society
eHST 12
WIYN Open Cluster Study. LXXXV. Li in NGC 2243: Implications for Stellar and Galactic Evolution
DOI: 10.3847/1538-3881/abe0b7 Bibcode: 2021AJ....161..159A

Twarog, Bruce A.; Anthony-Twarog, Barbara J.; Deliyannis, Constantine P.

High-dispersion spectra in the Li λ6708 region have been obtained and analyzed in the old, metal-deficient cluster NGC 2243. From Hydra spectra for 29 astrometric and radial velocity members, we derive rotational velocities, as well as [Fe/H], [Ca/H], [Si/H], and [Ni/H] based on 17, 1, 1, and 3 lines, respectively. Using ROBOSPECT, an automatic eq…

2021 The Astronomical Journal
Gaia 12
Runaway blue main-sequence stars at high Galactic latitudes. Target selection with Gaia and spectroscopic identification
DOI: 10.1051/0004-6361/202037872 Bibcode: 2021A&A...645A.108R

Raddi, Roberto; Irrgang, Andreas; Heber, Ulrich +2 more

Context. The ESA Gaia mission is a remarkable tool for stellar population analysis through its accurate Hertzsprung-Russell diagram. Its precise astrometry has propelled detailed kinematic studies of the Milky Way and the identification of high-velocity outliers.
Aims: Motivated by the historical identification of runaway main-sequence (MS) s…

2021 Astronomy and Astrophysics
Gaia 12
A new transient ultraluminous X-ray source in NGC 7090
DOI: 10.1093/mnras/staa3666 Bibcode: 2021MNRAS.501.1002W

Salvaterra, R.; Harrison, F. A.; Stern, D. +17 more

We report on the discovery of a new, transient ultraluminous X-ray source (ULX) in the galaxy NGC 7090. This new ULX, which we refer to as NGC 7090 ULX3, was discovered via monitoring with Swift during 2019-2020, and to date has exhibited a peak luminosity of LX ~ 6 × 1039 erg s-1. Archival searches show that, prio…

2021 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton eHST 12