activity
20082022
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 4k across the 59 of their papers we have counts for

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Showing 2015Show all

5 papers · 1 filter

astro-ph.SR2015★ 28 cited

From forced collapse to H ii region expansion in Mon R2: Envelope density structure and age determination with Herschel

P. Didelon, F. Motte, P. Tremblin +32

The surroundings of HII regions can have a profound influence on their development, morphology, and evolution. This paper explores the effect of the environment on H II regions in…

astro-ph.HE2015★ 40 cited

On gigahertz spectral turnovers in pulsars

Kaustubh Rajwade, Duncan R Lorimer, Loren D Anderson

Pulsars are known to emit non-thermal radio emission that is generally a power-law function of frequency. In some cases, a turnover is seen at frequencies around 100~MHz. Kijak et…

astro-ph.GA2015★ 21 cited

Untangling the Recombination Line Emission from HII Regions with Multiple Velocity Components

L. D. Anderson, L. A. Hough, T. V. Wenger +2

HII regions are the ionized spheres surrounding high-mass stars. They are ideal targets for tracing Galactic structure because they are predominantly found in spiral arms and have…

astro-ph.GA2015★ 63 cited

Bipolar HII regions - Morphology and star formation in their vicinity - I - G319.8800.79 and G010.3200.15

L. Deharveng, A. Zavagno, M. R. Samal +9

Our goal is to identify bipolar HII regions and to understand their morphology, their evolution, and the role they play in the formation of new generations of stars. We use the Spi…

astro-ph.GA2015

Azimuthal Metallicity Structure in the Milky Way Disk

Dana S. Balser, Trey V. Wenger, L. D. Anderson +1

Elemental abundance patterns in the Galactic disk constrain theories of the formation and evolution of the Milky Way. HII region abundances are the result of billions of years of c…