Search Publications

Von Zeipel - Lidov - Kozai cycles in action: Kepler triples with eclipse depth variations: KICs 6964043, 5653126, 5731312, and 8023317
DOI: 10.1093/mnras/stac1983 Bibcode: 2022MNRAS.515.3773B

Mitnyan, T.; Moe, M.; Toonen, S. +3 more

We report the results of the photodynamical analyses of four compact, tight triple stellar systems, KICs 6964043, 5653126, 5731312, and 8023317, based largely on Kepler and TESS data. All systems display remarkable eclipse timing and eclipse depth variations, the latter implying a non-aligned outer orbit. Moreover, KIC 6964043 is also a triply ecl…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
The post-common-envelope binary central star of the planetary nebula Ou 5: a doubly eclipsing post-red-giant-branch system
DOI: 10.1093/mnras/stab3736 Bibcode: 2022MNRAS.510.3102J

Corradi, Romano L. M.; Parsons, Steven G.; Munday, James +10 more

We present a detailed study of the stellar and orbital parameters of the post-common envelope binary central star of the planetary nebula Ou 5. Low-resolution spectra obtained during the primary eclipse - to our knowledge the first isolated spectra of the companion to a post-common-envelope planetary nebula central star - were compared to catalogu…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
The VMC survey - XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
DOI: 10.1093/mnras/stac712 Bibcode: 2022MNRAS.512.5423N

de Grijs, Richard; Ripepi, Vincenzo; Cioni, Maria-Rosa L. +7 more

We present proper motion (PM) measurements within the central region of the Large Magellanic Cloud (LMC), using near-infrared data from the VISTA survey of the Magellanic Cloud system (VMC). This work encompasses 18 VMC tiles covering a total sky area of ~28 deg2. We computed absolute stellar PMs from multiepoch observations in the K

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Deep diving off the 'Cosmic Cliffs': previously hidden outflows in NGC 3324 revealed by JWST
DOI: 10.1093/mnras/stac2820 Bibcode: 2022MNRAS.517.5382R

Smith, Nathan; Reiter, Megan; Morse, Jon A. +3 more

We present a detailed analysis of the protostellar outflow activity in the massive star-forming region NGC 3324, as revealed by new Early Release Observations (EROs) from the James Webb Space Telescope (JWST). Emission from numerous outflows is revealed in narrow-band images of hydrogen Paschen α (Paα) and molecular hydrogen. In particular, we rep…

2022 Monthly Notices of the Royal Astronomical Society
eHST JWST 15
Discovery of a coherent, wave-like velocity pattern for the Radcliffe wave
DOI: 10.1093/mnrasl/slac050 Bibcode: 2022MNRAS.517L.102L

Li, Guang-Xing; Chen, Bing-Qiu

Recent studies discovered that part of the Gould Belt belongs to a 2.7 kpc-long coherent, thin wave consisting of a chain of clouds, where a damped undulation pattern has been identified from the spatial arrangement of the clouds. We use the proper motions of young stellar objects anchored inside the clouds to study the kinematic structure of the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Inferring the rotation period distribution of stars from their projected rotation velocities and radii: Application to late-F/early-G Kepler stars
DOI: 10.1093/mnras/stab3650 Bibcode: 2022MNRAS.510.5623M

Petigura, Erik A.; Hall, Oliver J.; Masuda, Kento

While stellar rotation periods Prot may be measured from broad-band photometry, the photometric modulation becomes harder to detect for slower rotators, which could bias measurements of the long-period tail of the Prot distribution. Alternatively, the Prot distribution of stars can be inferred from their projected …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Local Group timing argument and virial theorem mass estimators from cosmological simulations
DOI: 10.1093/mnras/stac413 Bibcode: 2022MNRAS.511.6193H

Strigari, Louis E.; Hartl, Odelia V.

We identify Local Group (LG) analogues in the IllustrisTNG cosmological simulation, and use these to study two-mass estimators for the LG: One based on the timing argument (TA) and one based on the virial theorem (VT). Including updated measurements of the Milky Way-M31 tangential velocity and the cosmological constant, we show that the TA mass es…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Dark lenses through the dust: parallax microlensing events in the VVV
DOI: 10.1093/mnras/stac1507 Bibcode: 2022MNRAS.514.4845K

McGill, Peter; Smith, Leigh C.; Wyrzykowski, Łukasz +4 more

We use near-infrared photometry and astrometry from the VISTA Variables in the Via Lactea (VVV) survey to analyse microlensing events containing annual microlensing parallax information. These events are located in highly extincted and low-latitude regions of the Galactic bulge typically off-limits to optical microlensing surveys. We fit a catalog…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica
DOI: 10.1093/mnras/stac1383 Bibcode: 2022MNRAS.515.1328D

Triaud, Amaury H. M. J.; Quinn, Samuel N.; Stassun, Keivan G. +28 more

We report on the discovery and characterization of three planets orbiting the F8 star HD 28109, which sits comfortably in ${TESS}$'s continuous viewing zone. The two outer planets have periods of $\rm 56.0067 \pm 0.0003~d$ and $\rm 84.2597_{-0.0008}^{+0.0010}~d$, which implies a period ratio very close to that of the first-order 3:2 mean motion re…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
WIYN open cluster study: The old open cluster, NGC 188, and a re-evaluation of Lithium-richness among red giants
DOI: 10.1093/mnras/stac1251 Bibcode: 2022MNRAS.513.5387S

Cummings, Jeffrey D.; Twarog, Bruce A.; Anthony-Twarog, Barbara J. +3 more

We present WIYN1/Hydra spectra of 34 red giant candidate members of NGC 188, which, together with WOCS2 and Gaia data yield 23 single members, 6 binary members, 4 single non-members, and 1 binary non-member. We report [Fe/H] for 29 members and derive [Fe/H]NGC188 = +0.064 ± 0.018 dex (σµ) (sky spec…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15