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- Centre National de la Recherche ScientifiqueFR786 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR622 papers
- European Organization for Nuclear ResearchCH589 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT576 papers
- Lomonosov Moscow State UniversityRU562 papers
- University of OxfordGB556 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT551 papers
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- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di FrascatiIT528 papers
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15 papers · 2 filters
Subarcsecond international LOFAR radio images of the M82 nucleus at 118 MHz and 154 MHz
E. Varenius, J. E. Conway, I. Martí-Vidal +25
The nuclear starburst in the nearby galaxy M82 provides an excellent laboratory for understanding the physics of star formation. This galaxy has been extensively observed in the pa…
Herschel Far-Infrared Spectral-mapping of Orion BN/KL Outflows: Spatial distribution of excited CO, H2O, OH, O and C+ in shocked gas
Javier R. Goicoechea, Luis Chavarria, Jose Cernicharo +8
We present ~2'x2' spectral-maps of Orion BN/KL outflows taken with Herschel at ~12'' resolution. For the first time in the far-IR domain, we spatially resolve the emission associat…
Discovery of Carbon Radio Recombination Lines in M82
Leah K. Morabito, J. B. R. Oonk, Francisco Salgado +30
Carbon radio recombination lines (RRLs) at low frequencies (<=500 MHz) trace the cold, diffuse phase of the interstellar medium, which is otherwise difficult to observe. We present…
The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
B. Magnelli, R. J. Ivison, D. Lutz +21
[Abridged] We study the evolution of the radio spectral index and far-infrared/radio correlation (FRC) across the star-formation rate-stellar masse (i.e. SFR-M*) plane up to z 2. W…
The gas inflow and outflow rate in star-forming galaxies at
Kiyoto Yabe, Kouji Ohta, Masayuki Akiyama +5
We try to constrain the gas inflow and outflow rate of star-forming galaxies at by employing a simple analytic model for the chemical evolution of galaxies. The sample i…
Physical structure of the photodissociation regions in NGC 7023. Observations of gas and dust emission with Herschel
M. Köhler, E. Habart, H. Arab +16
The determination of the physical conditions in molecular clouds is a key step towards our understanding of their formation and evolution of associated star formation. We investiga…