Search Publications

LISA pathfinder appreciably constrains collapse models
DOI: 10.1103/PhysRevD.95.084054 Bibcode: 2017PhRvD..95h4054H

Slagmolen, B. J. J.; Helou, Bassam; McClelland, David E. +1 more

Spontaneous collapse models are phenomological theories formulated to address major difficulties in macroscopic quantum mechanics. We place significant bounds on the parameters of the leading collapse models, the continuous spontaneous localization (CSL) model, and the Diosi-Penrose (DP) model, by using LISA Pathfinder's measurement, at a record a…

2017 Physical Review D
LISAPathfinder 54
On the progenitor of the Type IIb supernova 2016gkg
DOI: 10.1093/mnras/stw3082 Bibcode: 2017MNRAS.465.4650K

Treu, Tommaso; Kilpatrick, Charles D.; Foley, Ryan J. +7 more

We present a detection in pre-explosion Hubble Space Telescope (HST) imaging of a point source consistent with being the progenitor star of the Type IIb supernova (SN IIb) 2016gkg. Post-explosion imaging from the Keck adaptive optics system was used to perform relative astrometry between the Keck and HST imaging. We identify a single point source …

2017 Monthly Notices of the Royal Astronomical Society
eHST 54
Evidence that the AGN dominates the radio emission in z ∼ 1 radio-quiet quasars
DOI: 10.1093/mnras/stx284 Bibcode: 2017MNRAS.468..217W

Jarvis, Matt J.; Kalfountzou, Eleni; White, Sarah V. +4 more

In order to understand the role of radio-quiet quasars (RQQs) in galaxy evolution, we must determine the relative levels of accretion and star-formation activity within these objects. Previous work at low radio flux densities has shown that accretion makes a significant contribution to the total radio emission, in contrast with other quasar studie…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 54
Luminous and Variable Stars in M31 and M33. IV. Luminous Blue Variables, Candidate LBVs, B[e] Supergiants, and the Warm Hypergiants: How to Tell Them Apart
DOI: 10.3847/1538-4357/aa582e Bibcode: 2017ApJ...836...64H

Humphreys, Roberta M.; Gordon, Michael S.; Martin, John C. +2 more

In this series of papers we have presented the results of a spectroscopic survey of luminous stars in the nearby spirals M31 and M33. Here, we present spectroscopy of 132 additional stars. Most have emission-line spectra, including luminous blue variables (LBVs) and candidate LBVs, Fe II emission line stars, the B[e] supergiants, and the warm hype…

2017 The Astrophysical Journal
eHST 54
Absolute Ages and Distances of 22 GCs Using Monte Carlo Main-sequence Fitting
DOI: 10.3847/1538-4357/aa6574 Bibcode: 2017ApJ...838..162O

Chaboyer, Brian; O'Malley, Erin M.; Gilligan, Christina

The recent Gaia Data Release 1 of stellar parallaxes provides ample opportunity to find metal-poor main-sequence stars with precise parallaxes. We select 21 such stars with parallax uncertainties better than σ π /π ≤ 0.10 and accurate abundance determinations suitable for testing metal-poor stellar evolution models and determining the …

2017 The Astrophysical Journal
Gaia eHST 54
Properties of the cosmological filament between two clusters: A possible detection of a large-scale accretion shock by Suzaku
DOI: 10.1051/0004-6361/201730497 Bibcode: 2017A&A...606A...1A

Kaastra, J. S.; Mernier, F.; Ishisaki, Y. +7 more

We report on the results of a Suzaku observation of the plasma in the filament located between the two massive clusters of galaxies, Abell 399 and Abell 401. Abell 399 (z = 0.0724) and Abell 401 (z = 0.0737) are expected to be in the initial phase of a cluster merger. In the region between the two clusters, we find a clear enhancement in the tempe…

2017 Astronomy and Astrophysics
Suzaku XMM-Newton 54
The Sirius System and Its Astrophysical Puzzles: Hubble Space Telescope and Ground-based Astrometry
DOI: 10.3847/1538-4357/aa6af8 Bibcode: 2017ApJ...840...70B

Schaefer, Gail H.; Bond, Howard E.; Burleigh, Matthew R. +11 more

Sirius, the seventh-nearest stellar system, is a visual binary containing the metallic-line A1 V star Sirius A, the brightest star in the sky, orbited in a 50.13 year period by Sirius B, the brightest and nearest white dwarf (WD). Using images obtained over nearly two decades with the Hubble Space Telescope (HST), along with photographic observati…

2017 The Astrophysical Journal
eHST 54
Sulfur dioxide in the Venus atmosphere: I. Vertical distribution and variability
DOI: 10.1016/j.icarus.2017.05.003 Bibcode: 2017Icar..295...16V

Vandaele, A. C.; Robert, S.; Montmessin, F. +18 more

Recent observations of sulfur containing species (SO2, SO, OCS, and H2SO4) in Venus' mesosphere have generated controversy and great interest in the scientific community. These observations revealed unexpected spatial patterns and spatial/temporal variability that have not been satisfactorily explained by models. S…

2017 Icarus
VenusExpress 54
Diamagnetic region(s): structure of the unmagnetized plasma around Comet 67P/CG
DOI: 10.1093/mnras/stx1540 Bibcode: 2017MNRAS.469S.372H

Glassmeier, K. -H.; Nilsson, H.; Carr, C. +14 more

The ESA's comet chaser Rosetta has monitored the evolution of the ionized atmosphere of comet 67P/Churyumov-Gerasimenko (67P/CG) and its interaction with the solar wind, during more than 2 yr. Around perihelion, while the cometary outgassing rate was highest, Rosetta crossed hundreds of unmagnetized regions, but did not seem to have crossed a larg…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 54
The PdBI Arcsecond Whirlpool Survey (PAWS): The Role of Spiral Arms in Cloud and Star Formation
DOI: 10.3847/1538-4357/836/1/62 Bibcode: 2017ApJ...836...62S

Leroy, Adam K.; Meidt, Sharon E.; Hughes, Annie +9 more

The process that leads to the formation of the bright star-forming sites observed along prominent spiral arms remains elusive. We present results of a multi-wavelength study of a spiral arm segment in the nearby grand-design spiral galaxy M51 that belongs to a spiral density wave and exhibits nine gas spurs. The combined observations of the (ioniz…

2017 The Astrophysical Journal
eHST 54