Search Publications

Dynamical masses and ages of Sirius-like systems
DOI: 10.1093/mnras/stad1849 Bibcode: 2023MNRAS.524..695Z

Kiman, Rocio; Brandt, Timothy D.; Li, Yiting +4 more

We measure precise orbits and dynamical masses and derive age constraints for six confirmed and one candidate Sirius-like systems, including the Hyades member HD 27483. Our orbital analysis incorporates radial velocities, relative astrometry, and Hipparcos-Gaia astrometric accelerations. We constrain the main-sequence lifetime of a white dwarf's p…

2023 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos eHST 6
Applying wavelet analysis to the X-ray light curves of active galactic nuclei and quasi-periodic eruptions
DOI: 10.1093/mnras/stad1955 Bibcode: 2023MNRAS.524.1478G

Gallo, L. C.; Gonzalez, A. G.; Ghosh, Akshay

In this work, we examine the application of the wavelet transform to the X-ray timing analyses of active galactic nuclei (AGN) and quasi-periodic eruption sources (QPEs). Several scenarios are simulated to test the effectiveness of the wavelet analysis to stationary and non-stationary data. We find that the power spectral density (PSD) slope and t…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 6
The spatial correlation of high-mass X-ray binaries and young star clusters in nearby star-forming galaxies
DOI: 10.1093/mnras/stad1368 Bibcode: 2023MNRAS.522.5669B

Williams, Benjamin F.; Binder, Breanna A.; Lazzarini, Margaret +2 more

We present an analysis of the two-point spatial correlation functions of high-mass X-ray binary (HMXB) and young star cluster (YSC) populations in M31 and M33. We find evidence that HMXBs are spatially correlated with YSCs to a higher degree than would be expected from random chance in both galaxies. When supplemented with similar studies in the M…

2023 Monthly Notices of the Royal Astronomical Society
eHST 6
HST PanCET programme: a flat optical transmission spectrum for the Hot Jupiter WASP-101b
DOI: 10.1093/mnras/stad1010 Bibcode: 2023MNRAS.522..582R

Mikal-Evans, Thomas; Sing, David K.; López-Morales, Mercedes +10 more

We present an optical transmission spectrum of the hot Jupiter WASP-101b. We observed three primary transits with Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph, covering a wavelength range from 0.3 to 1 $\mu$m. The observations suffer from significant systematics that we model using Gaussian Processes. Kernel selection for the …

2023 Monthly Notices of the Royal Astronomical Society
eHST 6
Chemical abundances of the Typhon stellar stream
DOI: 10.1093/mnras/stac2757 Bibcode: 2023MNRAS.519.4467J

Ting, Yuan-Sen; Naidu, Rohan P.; Simon, Joshua D. +2 more

We present the first high-resolution chemical abundances of seven stars in the recently discovered high-energy stream Typhon. Typhon stars have apocentres r ≳ 100 kpc, making this the first detailed chemical picture of the Milky Way's very distant stellar halo. Though the sample size is limited, we find that Typhon's chemical abundances are more l…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
Decoding the age-chemical structure of the Milky Way disc: an application of copulas and elicitable maps
DOI: 10.1093/mnras/stad2820 Bibcode: 2023MNRAS.526.1997P

Bovy, Jo; Frankel, Neige; Leung, Henry W. +2 more

In the Milky Way, the distribution of stars in the [α/Fe] versus [Fe/H] and [Fe/H] versus age planes holds essential information about the history of star formation, accretion, and dynamical evolution of the Galactic disc. We investigate these planes by applying novel statistical methods called copulas and elicitable maps to the ages and abundance…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
Morphologies and Central Stars of Planetary Nebulae in the Galactic bulge from VLT, HST and Pan-STARRS imaging
DOI: 10.1093/mnras/stac3490 Bibcode: 2023MNRAS.519.1049T

Parker, Quentin A.; Ritter, Andreas; Zijlstra, Albert +1 more

This is the first in a series of papers that present sets of different results for 136 compact, known planetary nebulae within a 10 × 10 degree region of the Galactic bulge. We use a large, previously unpublished sample of our own extensive ESO 8-m VLT deep imaging and spectroscopic data. This is combined with archival deep Hubble Space Telescope …

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 6
The role of tidal interactions in the formation of slowly rotating early-type stars in young star clusters
DOI: 10.1093/mnras/stad2674 Bibcode: 2023MNRAS.525.5880H

Wang, Li; de Grijs, Richard; Li, Chengyuan +9 more

The split main sequences found in the colour-magnitude diagrams of star clusters younger than ~600 Myr are suggested to be caused by the dichotomy of stellar rotation rates of upper main-sequence stars. Tidal interactions have been suggested as a possible explanation of the dichotomy of the stellar rotation rates. This hypothesis proposes that the…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
Isochrone fitting of Galactic globular clusters - V. NGC 6397 and NGC 6809 (M55)
DOI: 10.1093/mnras/stad3134 Bibcode: 2023MNRAS.526.5628G

Gontcharov, George A.; Mosenkov, Aleksandr V.; Khovritchev, Maxim Yu +8 more

We fit various colour-magnitude diagrams (CMDs) of the Galactic globular clusters NGC 6397 and NGC 6809 (M55) by isochrones from the Dartmouth Stellar Evolution Database (DSED) and Bag of Stellar Tracks and Isochrones (BaSTI) for α-enhanced [α/Fe] = +0.4. For the CMDs, we use data sets from Hubble Space Telescope, Gaia, Visible and Infrared Survey…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 6
UV-continuum β slopes of individual z 2-6 clumps and their evolution
DOI: 10.1093/mnras/stad3114 Bibcode: 2023MNRAS.526.5263B

Zanella, A.; Castellano, M.; Grillo, C. +11 more

We study the ultraviolet (UV) continuum β slope of a sample of 166 clumps, individual star-forming regions observed in high-redshift galaxies. They are hosted by 67 galaxies with redshift between 2 and 6.2, strongly lensed by the Hubble Frontier Fields cluster of galaxies MACS J0416.1 - 2403. The β slope is sensitive to a variety of physical prope…

2023 Monthly Notices of the Royal Astronomical Society
eHST 6