output
19962026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations

Showing 2012 · astro-ph.HEShow all

13 papers · 2 filters

astro-ph.HE2012★ 26 cited

High Frequency VLBI Rotation Measure of 8 AGN

J. C. Algaba

We have studied Very Long Baseline Array (VLBA) polarimetric observations of 8 sources including quasars and BL Lacs at 12, 15, 22, 24 and 43 GHz and high frequency rotation measur…

astro-ph.HE2012★ 426 cited

Jet Launching Structure Resolved Near the Supermassive Black Hole in M87

Sheperd S. Doeleman, Vincent L. Fish, David E. Schenck +30

Approximately 10% of active galactic nuclei exhibit relativistic jets, which are powered by accretion of matter onto super massive black holes. While the measured width profiles of…

astro-ph.HE2012★ 54 cited

Evolution of Post-Impact Companion Stars in SN Ia Remnants within the Single-Degenerate Scenario

Kuo-Chuan Pan, Paul Ricker, Ronald Taam

The nature of the progenitor systems of Type Ia supernovae is still uncertain. One way to distinguish between the single-degenerate scenario (SDS) and double-degenerate scenario (D…

astro-ph.HE2012★ 39 cited

Disk corona interaction: mechanism for the disk truncation and spectrum change in low luminosity AGN

Ronald E. Taam, B. F. Liu, W. Yuan +1

The truncation of an optically thick, geometrically thin accretion disk is investigated in the context of low luminosity AGN (LLAGN). We generalize the disk evaporation model used…

astro-ph.HE2012★ 7 cited

Launching and Quenching of Black Hole Relativistic Jets at Low Accretion Rate

Hung-Yi Pu, Kouichi Hirotani, Hsiang-Kuang Chang

Relativistic jets are launched from black hole (BH) X-ray binaries and active galactic nuclei when the disk accretion rate is below a certain limit (i.e., when the ratio of the acc…

astro-ph.HE2012★ 15 cited

Possible Detection of Apparent Superluminal inward motion in Markarian 421 after the Giant X-ray flare in February, 2010

K. Niinuma, M. Kino, H. Nagai +7

We report on the VLBI follow-up observations using the Japanese VLBI Network (JVN) array at 22 GHz for the largest X-ray flare of TeV blazar Mrk 421 that occurred in mid-February,…

astro-ph.HE2012★ 1k cited

Common Envelope Evolution: Where we stand and how we can move forward

N. Ivanova, S. Justham, X. Chen +16

This work aims to present our current best physical understanding of common-envelope evolution (CEE). We highlight areas of consensus and disagreement, and stress ideas which shoul…

astro-ph.HE2012★ 19 cited

Resolving the inner jet structure of 1924-292 with the EVENT HORIZON TELESCOPE

Ru-Sen Lu, Vincent L. Fish, Jonathan Weintroub +19

We present the first 1.3 mm (230 GHz) very long baseline interferometry model image of an AGN jet using closure phase techniques with a four-element array. The model image of the q…

astro-ph.HE2012★ 30 cited

Identifying the Location in the Host Galaxy of the Short GRB 111117A with the Chandra Sub-arcsecond Position

T. Sakamoto, E. Troja, K. Aoki +31

We present our successful Chandra program designed to identify, with sub-arcsecond accuracy, the X-ray afterglow of the short GRB 111117A, which was discovered by Swift and Fermi.…

astro-ph.HE2012★ 34 cited

VLBI and Single Dish Monitoring of 3C84 in the Period of 2009-2011

Hiroshi Nagai, Monica Orienti, Motoki Kino +13

The radio galaxy 3C 84 is a representative of gamma-ray-bright misaligned active galactic nuclei (AGNs) and one of the best laboratories to study the radio properties of the sub-pc…

astro-ph.HE2012★ 138 cited

Impact of type ia supernova ejecta on binary companions in the single-degenerate scenario

Kuo-Chuan Pan, Paul Ricker, Ronald Taam

Type Ia supernovae are thought to be caused by thermonuclear explosions of a carbon-oxygen white dwarf in close binary systems. In the single-degenerate scenario (SDS), the compani…

astro-ph.HE2012★ 12 cited

Energetic Fermi/LAT GRB100414A: Energetic and Correlations

Yuji Urata, Kuiyun Huang, Kazutaka Yamaoka +2

This study presents multi-wavelength observational results for energetic GRB100414A with GeV photons. The prompt spectral fitting using Suzaku/WAM data yielded spectral peak energi…

astro-ph.HE2012★ 17 cited

The GRB 071112C: A Case Study of Different Mechanisms in X-ray and Optical Temporal Evolution

K. Y. Huang, Y. Urata, Y. H. Tung +19

We present the study on GRB 071112C X-ray and optical light curves. In these two wavelength ranges, we have found different temporal properties. The R-band light curve showed an in…