Search Publications

Testing Dark Matter Halo Models of Quasars with Thermal Sunyaev-Zeldovich Effect
DOI: 10.1088/2041-8205/809/2/L32 Bibcode: 2015ApJ...809L..32C

Cen, Renyue; Safarzadeh, Mohammadtaher

A statistical analysis of stacked Compton-y maps of quasar hosts with a median redshift of 1.5 using Millennium Simulation is performed to address two issues: one on the feedback energy from quasars and the other on testing dark matter halo models for quasar hosts. On the first, we find that at the resolution of FWHM = 10 arcmin obtained by Planck…

2015 The Astrophysical Journal
Planck 21
When do stars in 47 Tucanae lose their mass?
DOI: 10.1088/0004-637X/810/2/127 Bibcode: 2015ApJ...810..127H

Marigo, Paola; Richer, Harvey B.; Heyl, Jeremy +4 more

By examining the diffusion of young white dwarfs through the core of the globular cluster 47 Tucanae, we estimate the time when the progenitor star lost the bulk of its mass to become a white dwarf. According to stellar evolution models of the white-dwarf progenitors in 47 Tucanae, we find this epoch to coincide approximately with the star ascendi…

2015 The Astrophysical Journal
eHST 21
The evolution of galaxy star formation activity in massive haloes
DOI: 10.1051/0004-6361/201424711 Bibcode: 2015A&A...574A.105P

Finoguenov, A.; Berta, S.; Magnelli, B. +20 more

Context. There is now a large consensus that the current epoch of the cosmic star formation history (CSFH) is dominated by low mass galaxies while the most active phase, between redshifts 1 and 2, is dominated by more massive galaxies, which evolve more quickly.
Aims: Massive galaxies tend to inhabit very massive haloes, such as galaxy groups…

2015 Astronomy and Astrophysics
Herschel 21
Magnetic Energy Dissipation during the 2014 March 29 Solar Flare
DOI: 10.1088/2041-8205/804/1/L20 Bibcode: 2015ApJ...804L..20A

Aschwanden, Markus J.

We calculated the time evolution of the free magnetic energy during the 2014 March 29 flare (SOL2014 March 29T17:48), the first X-class flare detected by the Interface Region Imaging Spectrograph (IRIS). The free energy was calculated from the difference between the nonpotential field, constrained by the geometry of observed loop structures, and t…

2015 The Astrophysical Journal
IRIS 21
Lower atmosphere minor gas abundances as retrieved from Venus Express VIRTIS-M-IR data at 2.3 µm
DOI: 10.1016/j.pss.2014.11.020 Bibcode: 2015P&SS..105..159H

Haus, Rainer; Kappel, David; Arnold, Gabriele

Minor gas abundances in the lower atmosphere of Venus' southern hemisphere are investigated using spectroscopic nightside measurements recorded by the Visible and InfraRed Thermal Imaging Spectrometer aboard ESA's Venus Express mission in the moderate spectral resolution infrared mapping channel (VIRTIS-M-IR, 1-5 µm, FWHM=17 nm). The entire …

2015 Planetary and Space Science
VenusExpress 21
Interchange Reconnection Forced by the Filament Eruption Inside a Pseudo-streamer
DOI: 10.1088/0004-637X/803/2/68 Bibcode: 2015ApJ...803...68Y

Yang, Jiayan; Bi, Yi; Hong, Junchao +2 more

We present rare observational signatures of interchange reconnection (IR) forced by the filament eruption inside a pseudo-streamer (PS). The PS was centered above a positive-polarity region bounded by two negative-polarity coronal holes (CHs), and thus its base contained two polarity inversion lines and a pair of loop arcades where two filaments w…

2015 The Astrophysical Journal
Hinode 21
IFU spectroscopy of 10 early-type galactic nuclei - III. Properties of the circumnuclear gas emission
DOI: 10.1093/mnras/stv1156 Bibcode: 2015MNRAS.451.3728R

Ricci, T. V.; Steiner, J. E.; Menezes, R. B.

Many early-type galaxies have ionized gas emission in their centres that extends to scales of ∼1 kpc. The majority of such objects are classified as low-ionization nuclear emission regions (LINERs), but the nature of their ionizing source is still not clear. The kinematics associated with these gaseous structures usually shows deviations from a pu…

2015 Monthly Notices of the Royal Astronomical Society
eHST 21
New insights into the evolution of the FR I radio galaxy 3C 270 (NGC 4261) from VLA and GMRT radio observations
DOI: 10.1093/mnras/stv665 Bibcode: 2015MNRAS.450.1732K

Raychaudhury, Somak; Giacintucci, Simona; Ishwara-Chandra, C. H. +4 more

We present the Giant Metrewave Radio Telescope 240 MHz observations of the nearby luminous Fanaroff-Riley type I radio source 3C 270, in the group-central elliptical NGC 4261. Combining these data with reprocessed Very Large Array 1.55 and 4.8 GHz observations, we produce spectral-index maps that reveal a constant spectral index along the jets and…

2015 Monthly Notices of the Royal Astronomical Society
XMM-Newton 21
The Transient Accreting X-Ray Pulsar XTE J1946+274: Stability of X-Ray Properties at Low Flux and Updated Orbital Solution
DOI: 10.1088/0004-637X/815/1/44 Bibcode: 2015ApJ...815...44M

Enoto, Teruaki; Terada, Yukikatsu; Hemphill, Paul B. +19 more

We present a timing and spectral analysis of the X-ray pulsar XTE J1946+274 observed with Suzaku during an outburst decline in 2010 October and compare with previous results. XTE J1946+274 is a transient X-ray binary consisting of a Be-type star and a neutron star with a 15.75 s pulse period in a 172 days orbit with 2-3 outbursts per orbit during …

2015 The Astrophysical Journal
INTEGRAL Suzaku 21
Anatomy of the AGN in NGC 5548. V. A clear view of the X-ray narrow emission lines
DOI: 10.1051/0004-6361/201526742 Bibcode: 2015A&A...581A..79W

Kaastra, J. S.; Kriss, G. A.; Bianchi, S. +15 more

Context. Our consortium performed an extensive multi-wavelength campaign of the nearby Seyfert 1 galaxy NGC 5548 in 2013-14. The source appeared unusually heavily absorbed in the soft X-rays, and signatures of outflowing absorption were also present in the UV. He-like triplets of neon, oxygen and nitrogen, and radiative recombination continuum (RR…

2015 Astronomy and Astrophysics
XMM-Newton 21