output
20022019
most citedFirst M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

4.3k citations

Showing 2015Show all

16 papers · 1 filter

astro-ph.GA2015158 cited

Star formation and the interstellar medium in z>6 UV-luminous Lyman-break galaxies

Chris J. Willott, Chris L. Carilli, Jeff Wagg +1

We present Atacama Large Millimeter Array (ALMA) detections of atomic carbon line and dust continuum emission in two UV-luminous galaxies at redshift 6. The far-infrared (FIR) lumi…

astro-ph.SR201524 cited

Time-variable non-thermal emission in the planetary nebula IRAS 15103-5754

Olga Suarez, Jose F. Gomez, Philippe Bendjoya +6

The beginning of photoionization marks the transition between the post-Asymptotic Giant Branch (post-AGB) and planetary nebula (PN) phases of stars with masses < 8 M_sun. This crit…

astro-ph.GA201539 cited

First Parallax Measurements Towards a 6.7 GHz Methanol Maser with the Australian Long Baseline Array - Distance to G339.884-1.259

V. Krishnan, S. P. Ellingsen, M. J. Reid +23

We have conducted the first parallax and proper motion measurements of 6.7 GHz methanol maser emission using the Australian Long Baseline Array (LBA). The parallax of G339.8841.…

astro-ph.SR2015101 cited

A Sub-arcsecond Survey Toward Class 0 Protostars in Perseus: Searching for Signatures of Protostellar Disks

John J. Tobin, Leslie W. Looney, David J. Wilner +7

We present a CARMA 1.3 mm continuum survey toward 9 Class 0 protostars in the Perseus molecular cloud at 0.3 (70 AU) resolution. This study approximately dou…

astro-ph.GA2015

Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect

Timothy Robishaw, James A. Green, Gabriele Surcis +12

The measurement of Zeeman splitting in spectral lines---both in emission and absorption---can provide direct estimates of the magnetic field strength and direction in atomic and mo…

astro-ph.HE201531 cited

Single pulse and profile variability study of PSR J1022+1001

K. Liu, R. Karuppusamy, K. J. Lee +6

Millisecond pulsars (MSPs) are known as highly stable celestial clocks. Nevertheless, recent studies have revealed the unstable nature of their integrated pulse profiles, which may…