about
The rarity of dust in metal-poor galaxies.PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas FractionsIonized and Molecular Gas Kinematics in a z = 1.4 Star-forming GalaxyLocal Swift-BAT active galactic nuclei prefer circumnuclear star formationThe Origins of [C ii] Emission in Local Star-forming GalaxiesThermal Pressure in the Cold Neutral Medium of Nearby GalaxiesThe spatially resolved [CII] cooling line deficit in galaxiesA multiwavelength exploration of the [C ii]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2The EDGE-CALIFA Survey: Interferometric Observations of 126 Galaxies with CARMAThe ionized gas in nearby galaxies as traced by the [N II] 122 and 205 {mu}m transitions[C II] 158 μm EMISSION AS A STAR FORMATION TRACERDust-to-gas ratio in the extremely metal-poor galaxy I Zw 18CARMA survey toward infrared-bright nearby galaxies (STING): molecular gas star formation law in NGC 4254The Origin of [C ii] 157 μm Emission in a Five-component Interstellar Medium: The Case of NGC 3184 and NGC 628Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby GalaxiesFirst Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C ii]-bright Gas and CO-bright Gas at Low MetallicityRotating Starburst Cores in Massive Galaxies at z = 2.5SHINING, A Survey of Far-infrared Lines in Nearby Galaxies. I. Survey Description, Observational Trends, and Line DiagnosticsSHINING, A Survey of Far-infrared Lines in Nearby Galaxies. II. Line-deficit Models, AGN Impact, [C ii]–SFR Scaling Relations, and Mass–Metallicity Relation in (U)LIRGsFar-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gasVALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35VALES. II. The physical conditions of interstellar gas in normal star-forming galaxies up to z = 0.2 revealed by ALMAInterstellar medium conditions in z ~ 0.2 Lyman-break analogsCARMA CO observations of three extremely metal-poor, star-forming galaxiesBulge-forming galaxies with an extended rotating disk at z ~ 2Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxiesVALES – III. The calibration between the dust continuum and interstellar gas content of star-forming galaxiesThe KMOS3D Survey: Demographics and Properties of Galactic Outflows at z = 0.6–2.7Kiloparsec Scale Properties of Star Formation Driven Outflows at z ∼ 2.3 in the SINS/zC-SINF AO SurveyMolecular and Ionized Gas Phases of an AGN-driven Outflow in a Typical Massive Galaxy at z ≈ 2
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P50
description
Chilean astrophysicist
@en
astrofísico chileno
@es
astrophysicien chilien
@fr
onderzoeker uit Chili
@nl
réaltfhisiceoir Sileach
@ga
name
Rodrigo Herrera Camus
@en
Rodrigo Herrera Camus
@ga
Rodrigo Herrera-Camus
@es
Rodrigo Herrera-Camus
@fr
Rodrigo Herrera-Camus
@nl
Rodrigo Herrera-Camus
@sl
type
label
Rodrigo Herrera Camus
@en
Rodrigo Herrera Camus
@ga
Rodrigo Herrera-Camus
@es
Rodrigo Herrera-Camus
@fr
Rodrigo Herrera-Camus
@nl
Rodrigo Herrera-Camus
@sl
altLabel
R. Herrera Camus
@en
R. Herrera-Camus
@en
Rodrigo Herrera-Camus
@en
prefLabel
Rodrigo Herrera Camus
@en
Rodrigo Herrera Camus
@ga
Rodrigo Herrera-Camus
@es
Rodrigo Herrera-Camus
@fr
Rodrigo Herrera-Camus
@nl
Rodrigo Herrera-Camus
@sl
P1412
P1950
P21
P27
P31
P496
0000-0002-2775-0595