about
COBE and the galactic interstellar medium: geometry of the spiral arms from FIR cooling linesFirst GLIMPSE Results on the Stellar Structure of the GalaxyDiscovery of interstellar CF⁺Ubiquitous argonium (ArH+) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gasHerschel PACS and SPIRE spectroscopy of the photodissociation regions associated with S 106 and IRAS 23133+6050The 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 galaxiesThe CO-to-H_2_ conversion factor and dust-to-gas ratio on kiloparsec scales in nearby galaxiesA study of heating and cooling of the ISM in NGC 1097 with Herschel-PACS and Spitzer-IRSHerschel far-infrared and submillimeter photometry for the KINGFISH sample of nearby galaxiesMapping the cold dust temperatures and masses of nearby KINGFISH galaxies with HerschelModeling dust and starlight in galaxies observed by Spitzer and Herschel: NGC 628 and NGC 6946Resolving the Far-IR line deficit: photoelectric heating and Far-IR line cooling in NGC 1097 and NGC 4559KINGFISH—Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image AtlasThe displaced dusty interstellar medium of NGC 3077: tidal stripping in the M 81 tripletEnhanced dust heating in the bulges of early-type spiral galaxiesFar-infrared line imaging of the starburst ring in NGC 1097 with the Herschel/PACS spectrometerMapping far-IR emission from the central kiloparsec of NGC 1097Mid‐Infrared IRS Spectroscopy of NGC 7331: A First Look at the Spitzer Infrared Nearby Galaxies Survey (SINGS) LegacyHeating and cooling of the neutral ISM in the NGC 4736 circumnuclear ringShock excited molecules in NGC 1266: ULIRG conditions at the center of a bulge-dominated galaxyThe emission by dust and stars of nearby galaxies in the Herschel KINGFISH surveyWarm Molecular Gas in M51: Mapping the Excitation Temperature and Mass of H2with theSpitzerInfrared SpectrographThe 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 TRACERThe Origin of [C ii] 157 μm Emission in a Five-component Interstellar Medium: The Case of NGC 3184 and NGC 628Physical conditions in the ionized gas of 30 DoradusFirst Results from the Herschel and ALMA Spectroscopic Surveys of the SMC: The Relationship between [C ii]-bright Gas and CO-bright Gas at Low MetallicityThe Stratospheric THz Observatory (STO)First Astronomical Detection of the CF + IonConstraints on the Cosmic-Ray Ionization Rate in the z ∼ 2.3 Lensed Galaxies SMM J2135–0102 and SDP 17b from Observations of OH+ and H2O+The [Cii] 158 Micron Line Deficit in Ultraluminous Infrared Galaxies RevisitedIdentification of Main‐Sequence Stars with Mid‐Infrared Excesses Using GLIMPSE: β Pictoris Analogs?Calculation of the Rate of the C⁺ + HF → CF⁺ + H Reaction: Implications for Fluorine Chemistry in the Interstellar MediumDisruption of the Orion molecular core 1 by wind from the massive star θ Orionis C
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description
American astrophysicist
@en
Amerikaans onderzoeker
@nl
astrofísico estadounidense
@es
astrophysicien américain
@fr
name
Mark Wolfire
@ast
Mark Wolfire
@en
Mark Wolfire
@es
Mark Wolfire
@fr
Mark Wolfire
@nl
Mark Wolfire
@sl
type
label
Mark Wolfire
@ast
Mark Wolfire
@en
Mark Wolfire
@es
Mark Wolfire
@fr
Mark Wolfire
@nl
Mark Wolfire
@sl
altLabel
M. G. Wolfire
@en
M. Wolfire
@en
prefLabel
Mark Wolfire
@ast
Mark Wolfire
@en
Mark Wolfire
@es
Mark Wolfire
@fr
Mark Wolfire
@nl
Mark Wolfire
@sl
P106
P1412
P21
P31
P496
0000-0003-0030-9510