activity
20012026
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 13.7k across the 324 of their papers we have counts for

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Showing 2013 · astro-ph.GAShow all

10 papers · 2 filters

astro-ph.GA2013★ 1 cited

Molecules in the Circumnuclear Disk of the Galactic Center

Nanase Harada, Denise Riquelme, Serena Viti +4

Within a few parsecs around the central Black Hole Sgr A*, chemistry in the dense molecular cloud material of the circumnuclear disk (CND) can be affected by many energetic phenome…

astro-ph.GA2013★ 60 cited

The CHESS survey of the L1157-B1 bow-shock: high and low excitation water vapor

G. Busquet, B. Lefloch, M. Benedettini +9

Molecular outflows powered by young protostars strongly affect the kinematics and chemistry of the natal molecular cloud through strong shocks resulting in substantial modification…

astro-ph.GA2013★ 40 cited

A combined IRAM and Herschel/HIFI study of cyano(di)acetylene in Orion KL: tentative detection of DC3N

G. B. Esplugues, J. Cernicharo, S. Viti +8

We present a study of cyanoacetylene (HC3N) and cyanodiacetylene (HC5N) in Orion KL, through observations from two line surveys performed with the IRAM 30m telescope and the HIFI i…

astro-ph.GA2013★ 52 cited

The B1 shock in the L1157 outflow as seen at high spatial resolution

M. Benedettini, S. Viti, C. Codella +7

We present high spatial resolution (750 AU at 250 pc) maps of the B1 shock in the blue lobe of the L1157 outflow in four lines: CS (3-2), CH3OH (3_K-2_K), HC3N (16-15) and p-H2CO (…

astro-ph.GA2013★ 16 cited

Broad N2H+ emission towards the protostellar shock L1157-B1

C. Codella, S. Viti, C. Ceccarelli +8

We present the first detection of N2H+ towards a low-mass protostellar outflow, namely the L1157-B1 shock, at about 0.1 pc from the protostellar cocoon. The detection was obtained…

astro-ph.GA2013★ 22 cited

A radical route to interstellar propylene formation

J. M. C. Rawlings, D. A. Williams, S. Viti +1

Complex organic molecules, such as propylene (CH3CHCH2), are detected in molecular clouds (such as TMC1) with high fractional abundances (~2.10^{-9}, relative to hydrogen) that can…

astro-ph.GA2013★ 25 cited

74 MHz Nonthermal Emission from Molecular Clouds: Evidence for a Cosmic Ray Dominated Region at the Galactic Center

F. Yusef-Zadeh, M. Wardle, D. Lis +5

We present 74 MHz radio continuum observations of the Galactic center region. These measurements show nonthermal radio emission arising from molecular clouds that is unaffected by…

astro-ph.GA2013★ 43 cited

Spatial distribution of small hydrocarbons in the neighborhood of the Ultra Compact HII region Monoceros R2

P. Pilleri, S. Treviño-Morales, A. Fuente +14

We study the chemistry of small hydrocarbons in the photon-dominated regions (PDRs) associated with the ultra-compact HII region Mon R2. Our goal is to determine the variations of…

astro-ph.GA2013★ 59 cited

Widespread Methanol Emission from the Galactic Center

F. Yusef-Zadeh, W. Cotton, S. Viti +2

We report the discovery of a widespread population of collisionally excited methanol J = 4_{-1} to 3$_0 E sources at 36.2 GHz from the inner 66'x18' (160x43 pc) of the Galactic cen…

astro-ph.GA2013★ 39 cited

Episodic Explosions in Interstellar Ices

J. M. C. Rawlings, D. A. Williams, S. Viti +1

We present a model for the formation of large organic molecules in dark clouds. The molecules are produced in the high density gas-phase that exists immediately after ice mantles a…