Search Publications

A new observational solar irradiance composite
DOI: 10.1002/2016JA023492 Bibcode: 2017JGRA..122.5910H

Schmutz, Werner; Haberreiter, Margit; Schöll, Micha +4 more

Variations in the solar spectral irradiance (SSI) are an important driver of the chemistry, temperature, and dynamics of the Earth's atmosphere and ultimately the Earth's climate. To investigate the detailed response of the Earth's atmosphere to SSI variations, a reliable SSI data set is needed. We present an observational SSI composite data set t…

2017 Journal of Geophysical Research (Space Physics)
SOHO 46
ALMA Observations of Starless Core Substructure in Ophiuchus
DOI: 10.3847/1538-4357/aa63f8 Bibcode: 2017ApJ...838..114K

Di Francesco, J.; Sadavoy, S. I.; Johnstone, D. +11 more

Compact substructure is expected to arise in a starless core as mass becomes concentrated in the central region likely to form a protostar. Additionally, multiple peaks may form if fragmentation occurs. We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 2 observations of 60 starless and protostellar cores in the Ophiuchus molecul…

2017 The Astrophysical Journal
Herschel 46
Space Motions of the Dwarf Spheroidal Galaxies Draco and Sculptor Based on HST Proper Motions with a ∼10 yr Time Baseline
DOI: 10.3847/1538-4357/aa917b Bibcode: 2017ApJ...849...93S

van der Marel, Roeland P.; van de Ven, Glenn; Bellini, Andrea +6 more

We present new proper motion (PM) measurements of the dwarf spheroidal galaxies (dSphs) Draco and Sculptor using multiepoch images obtained with the Hubble Space Telescope ACS/WFC. Our PM results have uncertainties far lower than previous measurements, even those made with the same instrument. The PM results for Draco and Sculptor are ({µ }<…

2017 The Astrophysical Journal
eHST 46
The late-time light curve of the Type Ia supernova SN 2011fe
DOI: 10.1093/mnras/stx683 Bibcode: 2017MNRAS.468.3798D

Gal-Yam, A.; Sullivan, M.; Nugent, P. +10 more

We present late-time optical R-band imaging data from the Palomar Transient Factory (PTF) for the nearby Type Ia supernova SN 2011fe. The stacked PTF light curve provides densely sampled coverage down to R ≃ 22 mag over 200-620 d past explosion. Combining with literature data, we estimate the pseudo-bolometric light curve for this event from 200 t…

2017 Monthly Notices of the Royal Astronomical Society
eHST 46
The independent pulsations of Jupiter's northern and southern X-ray auroras
DOI: 10.1038/s41550-017-0262-6 Bibcode: 2017NatAs...1..758D

Coates, A. J.; Jackman, C. M.; Jones, G. H. +14 more

Auroral hot spots are observed across the Universe at different scales1 and mark the coupling between a surrounding plasma environment and an atmosphere. Within our own Solar System, Jupiter possesses the only resolvable example of this large-scale energy transfer. Jupiter's northern X-ray aurora is concentrated into a hot spot, which i…

2017 Nature Astronomy
XMM-Newton 46
Improvement of solar-cycle prediction: Plateau of solar axial dipole moment
DOI: 10.1051/0004-6361/201731813 Bibcode: 2017A&A...607L...2I

Kusano, K.; Shiota, D.; Imada, S. +2 more


Aims: We report the small temporal variation of the axial dipole moment near the solar minimum and its application to the solar-cycle prediction by the surface flux transport (SFT) model.
Methods: We measure the axial dipole moment using the photospheric synoptic magnetogram observed by the Wilcox Solar Observatory (WSO), the ESA/NASA So…

2017 Astronomy and Astrophysics
SOHO 46
Diagnosing galactic feedback with line broadening in the low-redshift Lyα forest
DOI: 10.1093/mnrasl/slx004 Bibcode: 2017MNRAS.467L..86V

Viel, Matteo; Wakker, Bart P.; Kim, Tae-Sun +4 more

We compare the low-redshift (z ≃ 0.1) Lyα forest from hydrodynamical simulations with data from the Cosmic Origins Spectrograph. We find the tension between the observed number of lines with b-parameters in the range of 25-45 km s-1 and the predictions from simulations that incorporate either vigorous feedback from active galactic nucle…

2017 Monthly Notices of the Royal Astronomical Society
eHST 46
Super-Eddington QSO RX J0439.6-5311 - II. Multiwavelength constraints on the global structure of the accretion flow
DOI: 10.1093/mnras/stx1634 Bibcode: 2017MNRAS.471..706J

Done, Chris; Ward, Martin; Jin, Chichuan +1 more

We present a detailed multiwavelength study of an unobscured, highly super-Eddington Type-1 QSO RX J0439.6-5311. We combine the latest XMM-Newton observation with all archival data from infrared to hard X-rays. The optical spectrum is very similar to that of 1H 0707-495 in having extremely weak [O III] and strong Fe II emission lines, although the…

2017 Monthly Notices of the Royal Astronomical Society
IUE XMM-Newton eHST 46
Complexes of triggered star formation in supergiant shell of Holmberg II
DOI: 10.1093/mnras/stw2367 Bibcode: 2017MNRAS.464.1833E

Egorov, Oleg V.; Lozinskaya, Tatiana A.; Moiseev, Alexei V. +1 more

We report a detailed analysis of all regions of current star formation in the walls of the supergiant H I shell (SGS) in the galaxy Holmberg II based on observations with a scanning Fabry-Perot interferometer at the Russian 6-m telescope. We compare the structure and kinematics of ionized gas with that of atomic hydrogen and with the stellar popul…

2017 Monthly Notices of the Royal Astronomical Society
eHST 46
The large-scale nebular pattern of a superwind binary in an eccentric orbit
DOI: 10.1038/s41550-017-0060 Bibcode: 2017NatAs...1E..60K

Morris, Mark R.; Liu, Sheng-Yuan; Taam, Ronald E. +5 more

Preplanetary nebulae and planetary nebulae are evolved, mass-losing stellar objects that show a wide variety of morphologies. Many of these nebulae consist of outer structures that are nearly spherical (spiral/shell/arc/halo) and inner structures that are highly asymmetric (bipolar/multipolar) 1,2 . The coexistence of such geometrically…

2017 Nature Astronomy
eHST 46