Search Publications

The frequency and mass-ratio distribution of binaries in clusters - I. Description of the method and application to M67
DOI: 10.1093/mnras/stac1731 Bibcode: 2022MNRAS.515..730A

Albrow, Michael D.; Ulusele, Isaac H.

We present a new method for probabilistic generative modelling of stellar colour-magnitude diagrams (CMDs) to infer the frequency of binary stars and their mass-ratio distribution. The method invokes a mixture model to account for overlapping populations of single stars, binaries, and outliers in the CMD. We apply the model to Gaia observations of…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Evolution of the critical torus instability height and coronal mass ejection likelihood in solar active regions
DOI: 10.1051/0004-6361/202142910 Bibcode: 2022A&A...665A..37J

O'Kane, Jennifer; James, Alexander W.; Williams, David R.


Aims: Working towards improved space weather predictions, we aim to quantify how the critical height at which the torus instability drives coronal mass ejections (CMEs) varies over time in a sample of solar active regions.
Methods: We model the coronal magnetic fields of 42 active regions and quantify the critical height at their central…

2022 Astronomy and Astrophysics
SOHO 7
Is the Subsurface Meridional Flow Zero at the Equator?
DOI: 10.1007/s11207-022-02027-z Bibcode: 2022SoPh..297...99K

Komm, R.

We study the subsurface meridional flow and its divergence from the surface to a depth of about 16 Mm at the equator and its variation with the solar cycle derived with ring-diagram analysis applied to Michelson Doppler Imager (MDI) Dynamics Program, Global Oscillation Network Group (GONG), and Helioseismic and Magnetic Imager (HMI) Dopplergrams. …

2022 Solar Physics
SOHO 7
LoVoCCS. I. Survey Introduction, Data Processing Pipeline, and Early Science Results
DOI: 10.3847/1538-4357/ac68e8 Bibcode: 2022ApJ...933...84F

Cooper, M. C.; Donahue, Megan; Miyatake, Hironao +19 more

We present the Local Volume Complete Cluster Survey (LoVoCCS; we pronounce it as "low-vox" or "law-vox," with stress on the second syllable), an NSF's National Optical-Infrared Astronomy Research Laboratory survey program that uses the Dark Energy Camera to map the dark matter distribution and galaxy population in 107 nearby (0.03 < z < 0.12…

2022 The Astrophysical Journal
Gaia 7
The Twisted Magnetic Field of the Protobinary L483
DOI: 10.3847/1538-4357/ac722a Bibcode: 2022ApJ...932...34C

Pattle, Kate; Coudé, Simon; Bourke, Tyler L. +16 more

We present H-band (1.65 µm) and SOFIA HAWC+ 154 µm polarization observations of the low-mass core L483. Our H-band observations reveal a magnetic field that is overwhelmingly in the E-W direction, which is approximately parallel to the bipolar outflow that is observed in scattered IR light and in single-dish 12CO observation…

2022 The Astrophysical Journal
Gaia Herschel 7
Inconspicuous Solar Polar Coronal X-Ray Jets as the Source of Conspicuous Hinode/EUV Imaging Spectrometer Doppler Outflows
DOI: 10.3847/1538-4357/ac9960 Bibcode: 2022ApJ...940...85S

Harra, Louise K.; Panesar, Navdeep K.; Moore, Ronald L. +3 more

We examine in greater detail five events previously identified as being sources of strong transient coronal outflows in a solar polar region in Hinode/Extreme Ultraviolet (EUV) Imaging Spectrometer (EIS) Doppler data. Although relatively compact or faint and inconspicuous in Hinode/X-ray Telescope (XRT) soft-X-ray (SXR) images and in Solar Dynamic…

2022 The Astrophysical Journal
Hinode 7
Exploring the Link between the X-Ray Power Spectra and Energy Spectra of Active Galactic Nuclei
DOI: 10.3847/1538-4357/ac83bb Bibcode: 2022ApJ...936...36Y

Jin, Chichuan; Yuan, Weimin; Yang, Haonan

Active galactic nuclei (AGN) are generally considered the scaled-up counterparts of X-ray binaries (XRBs). It is known that the power spectral density (PSD) of the X-ray emission of XRBs shows significant evolution with spectral state. It is not clear whether AGN follow a similar evolutionary trend, however, though their X-ray emission and the PSD…

2022 The Astrophysical Journal
XMM-Newton 7
Searching for Variable Stars in the Open Cluster NGC 2355 and Its Surrounding Region
DOI: 10.3847/1538-3881/ac755a Bibcode: 2022AJ....164...40W

Hu, Qingshun; Zhang, Yu; Qin, Mingfeng +4 more

We have investigated the variable stars in the field surrounding NGC 2355 based on the time-series photometric observation data. More than 3000 CCD frames were obtained in the V band spread over 13 nights with the Nanshan One-meter Wide-field Telescope. We have detected 88 variable stars, containing 72 new variable stars and 16 known variable star…

2022 The Astronomical Journal
Gaia 7
Spectroscopic confirmation of a gravitationally lensed Lyman-break galaxy at z[C II] = 6.827 using NOEMA
DOI: 10.1093/mnras/stac557 Bibcode: 2022MNRAS.512..535M

Schaerer, D.; Zitrin, A.; van der Werf, P. +8 more

We present the spectroscopic confirmation of the brightest known gravitationally lensed Lyman-break galaxy in the Epoch of Reionization (EoR), A1703-zD1, through the detection of [C II] 158 $\mu$m at a redshift of z = 6.8269 ± 0.0004. This source was selected behind the strong lensing cluster Abell 1703, with an intrinsic luminosity and a very blu…

2022 Monthly Notices of the Royal Astronomical Society
eHST 7
Revising Properties of Planet-Host Binary Systems. I. Methods and Pilot Study
DOI: 10.3847/1538-4357/ac7be9 Bibcode: 2022ApJ...935..141S

Kraus, Adam L.; Mann, Andrew W.; Sullivan, Kendall

To fully leverage the statistical strength of the large number of planets found by projects such as the Kepler survey, the properties of planets and their host stars must be measured as accurately as possible. One key population for planet demographic studies is circumstellar planets in close binaries (ρ < 50 au), where the complex dynamical en…

2022 The Astrophysical Journal
Gaia 7