Search Publications

A detailed non-LTE analysis of LB-1: Revised parameters and surface abundances
DOI: 10.1051/0004-6361/201937318 Bibcode: 2020A&A...634L...7S

Allende Prieto, C.; Smartt, S. J.; Dufton, P. L. +8 more

Context. It has recently been proposed that LB-1 is a binary system at 4 kpc consisting of a B-type star of 8 M and a massive stellar black hole (BH) of 70 M. This finding challenges our current theories of massive star evolution and formation of BHs at solar metallicity.
Aims: Our objective is to derive the effective …

2020 Astronomy and Astrophysics
Gaia 30
Observations of the 2019 April 4 Solar Energetic Particle Event at the Parker Solar Probe
DOI: 10.3847/1538-4365/ab5712 Bibcode: 2020ApJS..246...35L

Krimigis, S. M.; Mitchell, D. G.; McComas, D. J. +33 more

A solar energetic particle event was detected by the Integrated Science Investigation of the Sun (IS⊙IS) instrument suite on Parker Solar Probe (PSP) on 2019 April 4 when the spacecraft was inside of 0.17 au and less than 1 day before its second perihelion, providing an opportunity to study solar particle acceleration and transport unprecedentedly…

2020 The Astrophysical Journal Supplement Series
SOHO 30
Recipes for bolometric corrections and Gaia luminosities of B-type stars: application to an asteroseismic sample
DOI: 10.1093/mnras/staa1292 Bibcode: 2020MNRAS.495.2738P

Aerts, Conny; Escorza, Ana; Pedersen, May G. +1 more

We provide three statistical model prescriptions for the bolometric corrections appropriate for B-type stars as a function of (I) Teff, (II) Teff and log g, and (III)Teff, log g and [M/H]. These statistical models have been calculated for 27 different filters, including those of the Gaia space mission, and were der…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
From Nuclear to Circumgalactic: Zooming in on AGN-driven Outflows at z ∼ 2.2 with SINFONI
DOI: 10.3847/1538-4357/ab86ad Bibcode: 2020ApJ...894...28D

Lutz, D.; Wuyts, S.; Förster Schreiber, N. M. +16 more

We use deep adaptive optics assisted integral field spectroscopy from SINFONI on the VLT to study the spatially resolved properties of ionized gas outflows driven by active galactic nuclei (AGNs) in three galaxies at z ∼ 2.2—K20-ID5, COS4-11337, and J0901 + 1814. These systems probe AGN feedback from nuclear to circumgalactic scales and provide un…

2020 The Astrophysical Journal
Gaia eHST 30
Classifying Single Stars and Spectroscopic Binaries Using Optical Stellar Templates
DOI: 10.3847/1538-4365/aba1e7 Bibcode: 2020ApJS..249...34R

Roulston, Benjamin R.; Green, Paul J.; Kesseli, Aurora Y.

Stellar spectral classification is a fundamental tool of modern astronomy, providing insight into physical characteristics such as effective temperature, surface gravity, and metallicity. Accurate and fast spectral typing is an integral need for large all-sky spectroscopic surveys like the Sloan Digital Sky Survey (SDSS) and the Large Sky Area Mul…

2020 The Astrophysical Journal Supplement Series
Gaia 30
Evolved massive stars at low metallicity. II. Red supergiant stars in the Small Magellanic Cloud
DOI: 10.1051/0004-6361/201937168 Bibcode: 2020A&A...639A.116Y

Yang, Ming; Bonanos, Alceste Z.; Jiang, Bi-Wei +9 more

We present the most comprehensive red supergiant (RSG) sample for the Small Magellanic Cloud (SMC) to date, including 1239 RSG candidates. The initial sample was derived based on a source catalog for the SMC with conservative ranking. Additional spectroscopic RSGs were retrieved from the literature, and RSG candidates were selected based on the in…

2020 Astronomy and Astrophysics
Gaia 30
The SUrvey for Pulsars and Extragalactic Radio Bursts - IV. Discovery and polarimetry of a 12.1-s radio pulsar
DOI: 10.1093/mnras/staa321 Bibcode: 2020MNRAS.493.1165M

Ray, P. S.; Kramer, M.; Johnston, S. +19 more

We report the discovery of PSR J2251-3711, a radio pulsar with a spin period of 12.1 s, the second longest currently known. Its timing parameters imply a characteristic age of 15 Myr, a surface magnetic field of 1.3 × 1013 G, and a spin-down luminosity of 2.9 × 1029 erg s-1. Its dispersion measure of 12.12(1) pc cm…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 30
Global helium abundance measurements in the solar corona
DOI: 10.1038/s41550-020-1156-6 Bibcode: 2020NatAs...4.1134M

Telloni, Daniele; Antonucci, Ester; Fineschi, Silvano +24 more

Solar abundances have been historically assumed to be representative of cosmic abundances. However, our knowledge of the solar abundance of helium, the second most abundant element, relies mainly on models1 and indirect measurements through helioseismic observations2, because actual measurements of helium in the solar atmosph…

2020 Nature Astronomy
SOHO 30
Core-collapse supernovae in binaries as the origin of galactic hyper-runaway stars
DOI: 10.1093/mnras/staa2334 Bibcode: 2020MNRAS.497.5344E

Rossi, E. M.; Renzo, M.; Evans, F. A.

Several stars detected moving at velocities near to or exceeding the Galactic escape speed likely originated in the Milky Way disc. We quantitatively explore the 'binary supernova scenario' hypothesis, wherein these 'hyper-runaway' stars are ejected at large peculiar velocities when their close, massive binary companions undergo a core-collapse su…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 30
MKT J170456.2-482100: the first transient discovered by MeerKAT
DOI: 10.1093/mnras/stz3027 Bibcode: 2020MNRAS.491..560D

Heywood, I.; Wijers, R. A. M. J.; Woudt, P. A. +19 more

We report the discovery of the first transient with MeerKAT, MKT J170456.2-482100, discovered in ThunderKAT images of the low-mass X-ray binary GX339-4. MKT J170456.2-482100 is variable in the radio, reaching a maximum flux density of 0.71± 0.11 mJy on 2019 October 12, and is undetected in 15 out of 48 ThunderKAT epochs. MKT J170456.2-482100 is co…

2020 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 30