Search Publications

Evidence for magnetic field compression in shocks within the jet of V404 Cyg
DOI: 10.1093/mnras/stw2171 Bibcode: 2016MNRAS.463.1822S

Covino, S.; Russell, D. M.; Fender, R. P. +3 more

We present optical and near-IR linear polarimetry of V404 Cyg during its 2015 outburst and in quiescence. We obtained time-resolved r'-band polarimetry when the source was in outburst, near-IR polarimetry when the source was near quiescence and multiple waveband optical polarimetry later in quiescence. The optical-to-near-IR linear pola…

2016 Monthly Notices of the Royal Astronomical Society
INTEGRAL 34
Planck Cold Clumps in the λ Orionis Complex. I. Discovery of an Extremely Young Class 0 Protostellar Object and a Proto-brown Dwarf Candidate in the Bright-rimmed Clump PGCC G192.32-11.88
DOI: 10.3847/0067-0049/222/1/7 Bibcode: 2016ApJS..222....7L

Sanhueza, Patricio; Kwon, Woojin; Lai, Shih-Ping +37 more

We are performing a series of observations with ground-based telescopes toward Planck Galactic cold clumps (PGCCs) in the λ Orionis complex in order to systematically investigate the effects of stellar feedback. In the particular case of PGCC G192.32-11.88, we discovered an extremely young Class 0 protostellar object (G192N) and a proto-brown dwar…

2016 The Astrophysical Journal Supplement Series
Planck 34
The Grism Lens-Amplified Survey from Space (GLASS). VII. The Diversity of the Distribution of Star Formation in Cluster and Field Galaxies at 0.3 less than or equal to z less than or equal to 0.7
DOI: 10.3847/1538-4357/833/2/178 Bibcode: 2016ApJ...833..178V

Pentericci, Laura; Schmidt, Kasper B.; Treu, Tommaso +10 more

Exploiting the slitless spectroscopy taken as part of the Grism Lens-Amplified Survey from Space (GLASS), we present an extended analysis of the spatial distribution of star formation in 76 galaxies in 10 clusters at 0.3\lt z\lt 0.7. We use 85 foreground and background galaxies in the same redshift range as a field sample. The samples are well mat…

2016 The Astrophysical Journal
eHST 34
Photospheric and coronal magnetic fields in six magnetographs. I. Consistent evolution of the bashful ballerina
DOI: 10.1051/0004-6361/201628096 Bibcode: 2016A&A...591A..78V

Mursula, Kalevi; Virtanen, Ilpo


Aims: We study the long-term evolution of photospheric and coronal magnetic fields and the heliospheric current sheet (HCS), especially its north-south asymmetry. Special attention is paid to the reliability of the six data sets used in this study and to the consistency of the results based on these data sets.
Methods: We use synoptic ma…

2016 Astronomy and Astrophysics
SOHO 34
Revealing the broad iron Kα line in Cygnus X-1 through simultaneous XMM-Newton, RXTE, and INTEGRAL observations
DOI: 10.1051/0004-6361/201424740 Bibcode: 2016A&A...589A..14D

Grinberg, Victoria; Pottschmidt, Katja; Staubert, Rüdiger +15 more

We report on the analysis of the broad Fe Kα line feature of Cyg X-1 in the spectra of four simultaneous hard intermediate state observations made with the X-ray Multiple Mirror mission (XMM-Newton), the Rossi X-ray Timing Explorer (RXTE), and the International Gamma-Ray Astrophysics Laboratory (INTEGRAL). The high quality of the XMM-Newton data t…

2016 Astronomy and Astrophysics
INTEGRAL XMM-Newton 34
A Microfilament-eruption Mechanism for Solar Spicules
DOI: 10.3847/2041-8205/828/1/L9 Bibcode: 2016ApJ...828L...9S

Moore, Ronald L.; Sterling, Alphonse C.

Recent investigations indicate that solar coronal jets result from eruptions of small-scale chromospheric filaments, called minifilaments; that is, the jets are produced by scaled-down versions of typical-sized filament eruptions. We consider whether solar spicules might in turn be scaled-down versions of coronal jets, being driven by eruptions of…

2016 The Astrophysical Journal
Hinode 34
Scale heights and equivalent widths of the iron K-shell lines in the Galactic diffuse X-ray emission
DOI: 10.1093/pasj/psw057 Bibcode: 2016PASJ...68...59Y

Koyama, Katsuji; Nobukawa, Masayoshi; Uchiyama, Hideki +2 more

This paper reports the analysis of the X-ray spectra of the Galactic diffuse X-ray emission (GDXE) in the Suzaku archive. The fluxes of the Fe I Kα (6.4 keV), Fe XXV Heα (6.7 keV), and Fe XXVI Lyα (6.97 keV) lines are separately determined. From the latitude distributions, we confirm that the GDXE is decomposed into the Galactic center (GCXE), the…

2016 Publications of the Astronomical Society of Japan
Suzaku 34
Far-infrared study of tracers of oxygen chemistry in diffuse clouds
DOI: 10.1051/0004-6361/201526473 Bibcode: 2016A&A...585A..76W

Menten, K. M.; Neufeld, D. A.; Stutzki, J. +8 more

Context. The chemistry of the diffuse interstellar medium rests upon three pillars: exothermic ion-neutral reactions ("cold chemistry"), endothermic neutral-neutral reactions with significant activation barriers ("warm chemistry"), and reactions on the surfaces of dust grains. While warm chemistry becomes important in the shocks associated with tu…

2016 Astronomy and Astrophysics
Herschel 34
Free-free and H42α emission from the dusty starburst within NGC 4945 as observed by ALMA
DOI: 10.1093/mnras/stw1659 Bibcode: 2016MNRAS.463..252B

Dickinson, C.; Bendo, G. J.; Karim, A. +3 more

We present observations of the 85.69 GHz continuum emission and H42α line emission from the central 30 arcsec within NGC 4945. Both sources of emission originate from nearly identical structures that can be modelled as exponential discs with scalelengths of ∼2.1 arcsec (or ∼40 pc). An analysis of the spectral energy distribution based on combining…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 34
The Vertical-current Approximation Nonlinear Force-free Field Code—Description, Performance Tests, and Measurements of Magnetic Energies Dissipated in Solar Flares
DOI: 10.3847/0067-0049/224/2/25 Bibcode: 2016ApJS..224...25A

Aschwanden, Markus J.

In this work we provide an updated description of the Vertical-Current Approximation Nonlinear Force-Free Field (VCA-NLFFF) code, which is designed to measure the evolution of the potential, non-potential, free energies, and the dissipated magnetic energies during solar flares. This code provides a complementary and alternative method to existing …

2016 The Astrophysical Journal Supplement Series
IRIS 34