activity
20072026
most citedRadio to gamma-ray variability study of blazar S5 0716+714

116 citations · 1.6k across the 50 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2025

The circumstellar environment around the extreme Galactic red supergiant NML Cygni: Dense, dusty, and asymmetric

E. De Beck, H. Andrews, G. Quintana-Lacaci +1

Supernova observations imply the presence of a dense and asymmetric circumstellar environment around SN Type II progenitors, whereas the mass loss from these progenitors, namely, r…

astro-ph.GA2022★ 9 cited

First detection of silicon-bearing molecules in Car

C. Bordiu, J. R. Rizzo, F. Bufano +11

We present ALMA band 6 observations of the luminous blue variable Eta Car, obtained within the ALMAGAL program. We report SiO J=5-4, SiS J=12-11 and SiN N=5-4 emission in the equat…

astro-ph.GA2022★ 9 cited

Dissecting the central regions of OH 231.8 + 4.2 with ALMA: a salty rotating disk at the base of a young bipolar outflow

C. Sánchez Contreras, J. Alcolea, R. Rodríguez Cardoso +5

We present ALMA continuum and molecular line emission maps at 1 mm of OH 231.8, a well studied bipolar nebula around an AGB star. The excellent angular resolution of our maps…

astro-ph.GA2017★ 12 cited

Clues to NaCN formation

G. Quintana-Lacaci, J. Cernicharo, L. Velilla Prieto +5

ALMA is providing us essential information on where certain molecules form. Observing where these molecules emission arises from, the physical conditions of the gas, and how this r…

astro-ph.GA2017★ 53 cited

IRC +10 216 in 3-D: morphology of a TP-AGB star envelope

M. Guélin, N. A. Patel, M. Bremer +10

During their late pulsating phase, AGB stars expel most of their mass in the form of massive dusty envelopes, an event that largely controls the composition of interstellar matter.…

astro-ph.GA2015★ 99 cited

Discovery of SiCSi in IRC+10216: A missing link between gas and dust carriers of SiC bonds

J. Cernicharo, M. C. McCarthy, C. A. Gottlieb +13

We report the discovery in space of a disilicon species, SiCSi, from observations between 80 and 350 GHz with the IRAM 30m radio telescope. Owing to the close coordination between…

astro-ph.GA2014★ 42 cited

New N-bearing species towards OH231.8+4.2: HNCO, HNCS, HCN and NO

L. Velilla Prieto, C. Sánchez Contreras, J. Cernicharo +7

OH231.8+4.2 is a well studied O-rich CSE around an intermediate-mass evolved star that displays bipolar molecular outflows accelerated up to 400 km/s. OH231 also presents an except…

astro-ph.GA2012★ 37 cited

Dense Gas in M33 (HerM33es)

C. Buchbender, C. Kramer, M. Gonzalez-Garcia +13

We aim to better understand the emission of molecular tracers of the diffuse and dense gas in giant molecular clouds and the influence that metallicity, optical extinction, density…

astro-ph.GA2012★ 23 cited

Herschel/HIFI observations of red supergiants and yellow hypergiants: I. Molecular inventory

D. Teyssier, G. Quintana-Lacaci, A. P. Marston +17

Red supergiant stars (RSGs) and yellow hypergiant stars (YHGs) are believed to be the high-mass counterparts of stars in the AGB and early post-AGB phases. We study the mass-loss i…

astro-ph.GA2011★ 49 cited

The Herschel M33 extended survey (HerM33es): PACS spectroscopy of the star forming region BCLMP 302

B. Mookerjea, C. Kramer, C. Buchbender +19

Context: The emission line of [CII] at 158 micron is one of the strongest cooling lines of the interstellar medium (ISM) in galaxies. Aims: Disentangling the relative contributions…