Search Publications

The Magellan/PFS Exoplanet Search: a 55-d period dense Neptune transiting the bright (V = 8.6) star HD 95338
DOI: 10.1093/mnras/staa1724 Bibcode: 2020MNRAS.496.4330D

Butler, R. Paul; Kane, Stephen R.; Crane, Jeffrey D. +14 more

We report the detection of a transiting, dense Neptune planet candidate orbiting the bright (V = 8.6) K0.5V star HD 95338. Detection of the 55-d periodic signal comes from the analysis of precision radial velocities from the Planet Finder Spectrograph on the Magellan II Telescope. Follow-up observations with HARPS also confirm the presence of the …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
The Population of Galactic Planetary Nebulae: a Study of Distance Scales and Central Stars Based on the Second Gaia Release
DOI: 10.3847/1538-4357/ab59e4 Bibcode: 2020ApJ...889...21S

Stanghellini, Letizia; Bucciarelli, Beatrice; Lattanzi, Mario G. +1 more

We matched the astrometry of central stars (CSs) of spectroscopically confirmed Galactic planetary nebulae (PNe) with DR2 Gaia parallaxes (p), finding 430 targets in common with p > 0 and $| {\sigma }_{{\rm{p}}}/p| \lt 1$ ∣ σ p / p ∣ < 1 . A catalog of PNe whose CSs have DR2 Gaia parallaxes is presented in Table 1. We compared DR2 parallaxes…

2020 The Astrophysical Journal
Gaia 20
Experimental Phase Function and Degree of Linear Polarization Curves of Millimeter-sized Cosmic Dust Analogs
DOI: 10.3847/1538-4365/ab6851 Bibcode: 2020ApJS..247...19M

Sierks, H.; Blum, J.; Fulle, M. +22 more

We present laboratory measurements of the phase functions and degree of linear polarization (DLP) curves of a selection of millimeter-sized cosmic dust analog particles. The set includes particles with similar sizes but diverse internal structure (compact and porous) and absorbing properties. The measured phase functions are found to be in all cas…

2020 The Astrophysical Journal Supplement Series
Rosetta 20
TESS observations of southern ultrafast rotating low-mass stars
DOI: 10.1093/mnras/staa2021 Bibcode: 2020MNRAS.497.2320R

Ramsay, Gavin; Doyle, Lauren; Doyle, J. Gerry

In our previous study of low-mass stars using TESS, we found a handful that show a periodic modulation on a period <1 d but also displayed no flaring activity. Here we present the results of a systematic search for ultrafast rotators (UFRs) in the Southern ecliptic hemisphere, which were observed in 2-min cadence with TESS. Using data from Gaia…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
Stellar occultations enable milliarcsecond astrometry for Trans-Neptunian objects and Centaurs
DOI: 10.1051/0004-6361/202039054 Bibcode: 2020A&A...644A..40R

Naletto, G.; Pál, A.; Snodgrass, C. +66 more

Context. Trans-Neptunian objects (TNOs) and Centaurs are remnants of our planetary system formation, and their physical properties have invaluable information for evolutionary theories. Stellar occultation is a ground-based method for studying these distant small bodies and has presented exciting results. These observations can provide precise pro…

2020 Astronomy and Astrophysics
Gaia 20
A statistical study of plasmoids associated with a post-CME current sheet
DOI: 10.1051/0004-6361/202039000 Bibcode: 2020A&A...644A.158P

Pant, Vaibhav; Banerjee, Dipankar; Patel, Ritesh +1 more

Context. Coronal mass ejections (CMEs) are often observed to be accompanied by flare, current sheets, and plasmoids/plasma blobs. 2D and 3D numerical simulations and observations reported plasmoids moving upward as well as downward along the current sheet.
Aims: We aim to investigate the properties of plasmoids observed in the current sheet f…

2020 Astronomy and Astrophysics
SOHO 20
Most EL CVn systems are inner binaries of hierarchical triples
DOI: 10.1093/mnrasl/slaa164 Bibcode: 2020MNRAS.499L.121L

Gänsicke, B. T.; Parsons, S. G.; Schreiber, M. R. +2 more

In spite of their importance for modern astronomy, we do not fully understand how close binary stars containing at least one white dwarf form from main-sequence binary stars. The discovery of EL CVn binaries, close pre-white dwarfs with A/F main-sequence star companions, offers now the unique possibility to test models of close compact binary star…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
Distribution of methanol and cyclopropenylidene around starless cores★
DOI: 10.1051/0004-6361/201936598 Bibcode: 2020A&A...643A..60S

Nagy, Z.; Caselli, P.; Spezzano, S. +3 more

Context. The spatial distribution of molecules around starless cores is a powerful tool for studying the physics and chemistry governing the earliest stages of star formation.
Aims: Our aim is to study the chemical differentiation in starless cores to determine the influence of large-scale effects on the spatial distribution of molecules with…

2020 Astronomy and Astrophysics
Herschel 20
K2 Ultracool Dwarfs Survey - VI. White light superflares observed on an L5 dwarf and flare rates of L dwarfs
DOI: 10.1093/mnras/staa1137 Bibcode: 2020MNRAS.494.5751P

Mullan, D. J.; Burgasser, A. J.; Gizis, J. E. +3 more

Kepler K2 long cadence data are used to study white light flares in a sample of 45 L dwarfs. We identified 11 flares on 9 L dwarfs with equivalent durations of (1.3-198) h and total (UV/optical/IR) energies of ≥0.9 × 1032 erg. Two superflares with energies of >1033 erg were detected on an L5 dwarf (VVV BD001): this is the …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
The 2019 eruption of recurrent nova V3890 Sgr: observations by Swift, NICER, and SMARTS
DOI: 10.1093/mnras/staa3083 Bibcode: 2020MNRAS.499.4814P

Ness, J. -U.; Orio, M.; Osborne, J. P. +6 more

V3890 Sgr is a recurrent nova that has been seen in outburst three times so far, with the most recent eruption occurring on 2019 August 27 UT. This latest outburst was followed in detail by the Neil Gehrels Swift Observatory, from less than a day after the eruption until the nova entered the Sun observing constraint, with a small number of additio…

2020 Monthly Notices of the Royal Astronomical Society
IUE XMM-Newton 20