Search Publications

A period-dependent spatial scatter of Galactic black hole transients
DOI: 10.1093/mnrasl/slaa081 Bibcode: 2020MNRAS.496L..22G

Maccarone, T. J.; Charles, P. A.; Gandhi, P. +4 more

There remain significant uncertainties in the origin and evolution of black holes in binary systems, in particular regarding their birth sites and the influence of natal kicks. These are long-standing issues, but their debate has been reinvigorated in the era of gravitational wave detections and the improving precision of astrometric measurements.…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
An ablating 2.6 M planet in an eccentric binary from the Dispersed Matter Planet Project
DOI: 10.1038/s41550-019-0972-z Bibcode: 2020NatAs...4..419B

Jenkins, James S.; Anglada-Escudé, Guillem; Díaz, Matías R. +8 more

Earth-mass exoplanets are difficult to detect. The Dispersed Matter Planet Project (DMPP) identifies stars that are likely to host the most detectable low-mass exoplanets. The star DMPP-3 (HD 42936) shows signs of circumstellar absorption, indicative of mass loss from ablating planets. Here, we report the radial velocity discovery of a highly ecce…

2020 Nature Astronomy
Gaia 20
The R-Process Alliance: A Very Metal-poor, Extremely r-process-enhanced Star with [Eu/Fe] = + 2.2, and the Class of r-III Stars
DOI: 10.3847/1538-4357/ab97ba Bibcode: 2020ApJ...898...40C

Beers, Timothy C.; Placco, Vinicius M.; Hattori, Kohei +8 more

We report the discovery of J1521-3538, a bright (V = 12.2), very metal-poor ([Fe/H] = -2.8) strongly r-process-enhanced field horizontal branch star, based on a high-resolution, high signal-to-noise Magellan/MIKE spectrum. J1521-3538 shows the largest r-process element overabundance in any known r-process-enhanced star, with [Eu/Fe] = +2.2, and it…

2020 The Astrophysical Journal
Gaia 20
Astrometric effects of gravitational wave backgrounds with nonluminal propagation speeds
DOI: 10.1103/PhysRevD.101.024038 Bibcode: 2020PhRvD.101b4038M

Gilmore, Gerard; Mihaylov, Deyan P.; Moore, Christopher J. +2 more

A passing gravitational wave causes a deflection in the apparent astrometric positions of distant stars. The effect of the speed of the gravitational wave on this astrometric shift is discussed. A stochastic background of gravitational waves would result in a pattern of astrometric deflections which are correlated on large angular scales. These co…

2020 Physical Review D
Gaia 20
Sixteen overlooked open clusters in the fourth Galactic quadrant. A combined analysis of UBVI photometry and Gaia DR2 with ASteCA
DOI: 10.1051/0004-6361/201937141 Bibcode: 2020A&A...637A..95P

Moitinho, A.; Carraro, G.; Perren, G. I. +3 more


Aims: This paper has two main objectives: (1) To determine the intrinsic properties of 16 faint and mostly unstudied open clusters in the poorly known sector of the Galaxy at 270° -300° to probe the Milky Way structure in future investigations. (2) To address previously reported systematics in Gaia DR2 parallaxes by comparing the cluster dist…

2020 Astronomy and Astrophysics
Gaia 20
The Accretion History of AGN: A Newly Defined Population of Cold Quasars
DOI: 10.3847/1538-4357/aba358 Bibcode: 2020ApJ...900....5K

Kartaltepe, Jeyhan S.; Kirkpatrick, Allison; Marchesi, Stefano +15 more

Quasars are the most luminous of active galactic nuclei, and are perhaps responsible for quenching star formation in their hosts. The Stripe 82X catalog covers 31.3 deg2 of the Stripe 82 field, of which the 15.6 deg2 covered with XMM-Newton is also covered by Herschel/SPIRE. We have 2500 X-ray detected sources with multiwavel…

2020 The Astrophysical Journal
Herschel XMM-Newton 20
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