Applied Optics, ISSN 1559-128X, 06/2013, Volume 52, Issue 16, pp. 3864 - 3875
One of the instruments on board the Herschel Space Observatory is the Spectral and Photometric Imaging Receiver (SPIRE). SPIRE employs a Fourier transform...
Astronomical instruments
Astronomical instruments
Journal Article
Nature, ISSN 0028-0836, 12/2016, Volume 540, Issue 7633, pp. 406 - 409
Young stars are associated with prominent outflows of molecular gas(1,2). The ejection of gas is believed to remove angular momentum from the protostellar...
ROTATION | TRANSITION | TAURI | MULTIDISCIPLINARY SCIENCES | YOUNG STARS | ENVELOPE | JET | CHONDRULES | FLOWS | Observations | Natural history | Protostars | Wind | Carbon monoxide | Solar systems | Stars & galaxies | Methods | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
ROTATION | TRANSITION | TAURI | MULTIDISCIPLINARY SCIENCES | YOUNG STARS | ENVELOPE | JET | CHONDRULES | FLOWS | Observations | Natural history | Protostars | Wind | Carbon monoxide | Solar systems | Stars & galaxies | Methods | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 11/2016, Volume 595, p. A117
Context. The inner regions of the envelopes surrounding young protostars are characterized by a complex chemistry, with prebiotic molecules present on the...
ISM: individual objects: IRAS 16293-2422 | Stars: protostars | Astrochemistry | Submillimeter: ISM | ISM: molecules | Stars: formation | stars: protostars | WATER DEUTERIUM FRACTIONATION | COMPLEX ORGANIC-MOLECULES | LOW-MASS PROTOSTAR | STAR-FORMING REGIONS | HOT-CORE | GRAIN-SURFACE-CHEMISTRY | YOUNG STELLAR OBJECTS | stars: formation | ETHYLENE-GLYCOL | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | astrochemistry | INTERSTELLAR HEAVY-WATER | Origins | Ethylene glycol | Star formation | Methyl alcohol | Radio telescopes | Deuteration | Protostars | Interferometry | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
ISM: individual objects: IRAS 16293-2422 | Stars: protostars | Astrochemistry | Submillimeter: ISM | ISM: molecules | Stars: formation | stars: protostars | WATER DEUTERIUM FRACTIONATION | COMPLEX ORGANIC-MOLECULES | LOW-MASS PROTOSTAR | STAR-FORMING REGIONS | HOT-CORE | GRAIN-SURFACE-CHEMISTRY | YOUNG STELLAR OBJECTS | stars: formation | ETHYLENE-GLYCOL | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | astrochemistry | INTERSTELLAR HEAVY-WATER | Origins | Ethylene glycol | Star formation | Methyl alcohol | Radio telescopes | Deuteration | Protostars | Interferometry | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2018, Volume 476, Issue 4, pp. 4949 - 4964
The evolutionary past of our Solar system can be pieced together by comparing analogous low-mass protostars with remnants of our Protosolar Nebula - comets....
Stars: protostars | ISM: molecule | Astrochemistry | Comets: general | CARBONYL SULFIDE OCS | stars: protostars | DIPOLE-MOMENT | ORGANOSULFUR CHEMISTRY | SUBMILLIMETER-WAVE SPECTRUM | ROTATIONAL SPECTRUM | MICROWAVE-SPECTRUM | MASS STAR-FORMATION | DENSE INTERSTELLAR CLOUDS | ISM: molecules | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | CENTRIFUGAL-DISTORTION | comets: general | astrochemistry | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | Other Basic Medicine | Analytical Chemistry | Astronomi, astrofysik och kosmologi | Annan medicinsk grundvetenskap | Analytisk kemi | Astronomy, Astrophysics and Cosmology
Stars: protostars | ISM: molecule | Astrochemistry | Comets: general | CARBONYL SULFIDE OCS | stars: protostars | DIPOLE-MOMENT | ORGANOSULFUR CHEMISTRY | SUBMILLIMETER-WAVE SPECTRUM | ROTATIONAL SPECTRUM | MICROWAVE-SPECTRUM | MASS STAR-FORMATION | DENSE INTERSTELLAR CLOUDS | ISM: molecules | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | CENTRIFUGAL-DISTORTION | comets: general | astrochemistry | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | Other Basic Medicine | Analytical Chemistry | Astronomi, astrofysik och kosmologi | Annan medicinsk grundvetenskap | Analytisk kemi | Astronomy, Astrophysics and Cosmology
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2015, Volume 801, Issue 2, pp. 1 - 18
(Ultra) luminous infrared galaxies ((U)LIRGs) are objects characterized by their extreme infrared (8-1000 mu m) luminosities (L-LIRG > 10(11) L-circle dot and...
galaxies: individual (ULIRGs) | photon-dominated region (PDR) | molecular data | galaxies: ISM | submillimeter: ISM | FOURIER-TRANSFORM SPECTROMETER | PHYSICAL CONDITIONS | DENSE MOLECULAR GAS | STAR-FORMATION | ACTIVE GALACTIC NUCLEI | WATER-VAPOR | SPACE-OBSERVATORY MEASUREMENTS | ARP 220 | ASTRONOMY & ASTROPHYSICS | MARKARIAN 231 | ULTRALUMINOUS INFRARED GALAXIES | Infrared | Galaxies | Heating | Emission | Luminosity | Space telescopes | Excitation | Ladders | Physics - Astrophysics of Galaxies | LUMINOSITY | TELESCOPES | EXCITATION | CAMERAS | FINE STRUCTURE | GAS COOLING | PHOTONS | HEATING | COMPARATIVE EVALUATIONS | CARBON MONOXIDE | SPACE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | INFRARED SPECTRA | LINE WIDTHS | SATELLITES | GALAXIES | GALAXY NUCLEI | FAR INFRARED RADIATION | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
galaxies: individual (ULIRGs) | photon-dominated region (PDR) | molecular data | galaxies: ISM | submillimeter: ISM | FOURIER-TRANSFORM SPECTROMETER | PHYSICAL CONDITIONS | DENSE MOLECULAR GAS | STAR-FORMATION | ACTIVE GALACTIC NUCLEI | WATER-VAPOR | SPACE-OBSERVATORY MEASUREMENTS | ARP 220 | ASTRONOMY & ASTROPHYSICS | MARKARIAN 231 | ULTRALUMINOUS INFRARED GALAXIES | Infrared | Galaxies | Heating | Emission | Luminosity | Space telescopes | Excitation | Ladders | Physics - Astrophysics of Galaxies | LUMINOSITY | TELESCOPES | EXCITATION | CAMERAS | FINE STRUCTURE | GAS COOLING | PHOTONS | HEATING | COMPARATIVE EVALUATIONS | CARBON MONOXIDE | SPACE | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | INFRARED SPECTRA | LINE WIDTHS | SATELLITES | GALAXIES | GALAXY NUCLEI | FAR INFRARED RADIATION | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2016, Volume 590, p. L6
Formamide (NH2CHO) has previously been detected in several star-forming regions and is thought to be a precursor for different prebiotic molecules. Its...
ISM: individual objects: IRAS 16293-2422 | Stars: protostars | Astrochemistry | ISM: molecules | Stars: formation | Astrobiology | stars: protostars | IRAS 16293-2422 | ROTATIONAL SPECTRUM | COLOGNE DATABASE | LOW-MASS PROTOSTAR | MICROWAVE-SPECTRUM | GRAIN-SURFACE-CHEMISTRY | stars: formation | astrobiology | 1 THZ | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | MOLECULAR-SPECTROSCOPY | astrochemistry | GAS-PHASE REACTIONS | Fractionation | Star formation | Images | Formations | Deuteration | Arrays | Standards | Protostars | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
ISM: individual objects: IRAS 16293-2422 | Stars: protostars | Astrochemistry | ISM: molecules | Stars: formation | Astrobiology | stars: protostars | IRAS 16293-2422 | ROTATIONAL SPECTRUM | COLOGNE DATABASE | LOW-MASS PROTOSTAR | MICROWAVE-SPECTRUM | GRAIN-SURFACE-CHEMISTRY | stars: formation | astrobiology | 1 THZ | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | MOLECULAR-SPECTROSCOPY | astrochemistry | GAS-PHASE REACTIONS | Fractionation | Star formation | Images | Formations | Deuteration | Arrays | Standards | Protostars | Astronomi, astrofysik och kosmologi | Astronomy, Astrophysics and Cosmology
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 440, Issue 4, pp. 3658 - 3674
The Herschel Spectral and Photometric REceiver (SPIRE) instrument consists of an imaging photometric camera and an imaging Fourier Transform Spectrometer...
Instrumentation: spectrographs | Space vehicles: instruments | Techniques: spectroscopic | THERMAL INERTIA | space vehicles: instruments | WAVELENGTHS | URANUS | PERFORMANCE | instrumentation: spectrographs | INSTRUMENT | SPECTROSCOPY | techniques: spectroscopic | MARS | ASTRONOMY & ASTROPHYSICS | CIRCUMSTELLAR ENVELOPES | BRIGHTNESS TEMPERATURE SPECTRA | NEAR-MILLIMETER | Physics - Instrumentation and Methods for Astrophysics | Sciences of the Universe | Astrophysics
Instrumentation: spectrographs | Space vehicles: instruments | Techniques: spectroscopic | THERMAL INERTIA | space vehicles: instruments | WAVELENGTHS | URANUS | PERFORMANCE | instrumentation: spectrographs | INSTRUMENT | SPECTROSCOPY | techniques: spectroscopic | MARS | ASTRONOMY & ASTROPHYSICS | CIRCUMSTELLAR ENVELOPES | BRIGHTNESS TEMPERATURE SPECTRA | NEAR-MILLIMETER | Physics - Instrumentation and Methods for Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 04/2018, Volume 612, p. A72
Context. The Class 0 protostellar binary IRAS 16293-2422 is an interesting target for (sub) millimeter observations due to, both, the rich chemistry toward the...
Stars: protostars | Astrochemistry | Submillimeter: ISM | ISM: molecules | Stars: formation | ISM: individual objects: IRAS 16293-2422 (except planetary nebulae) | ORGANIC-MOLECULES | stars: protostars | HOT CORE | STAR-FORMATION | ROTATIONAL SPECTRUM | SUBMILLIMETER ARRAY | INTERSTELLAR-MEDIUM | OPHIUCHUS | LOW-MASS PROTOSTARS | stars: formation | YOUNG | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | IRAS-16293-2422 | astrochemistry | Angular resolution | Temperature regions | One dimensional models | Radiation | Luminosity | Emission | Protoplanetary disk | Density | Protostars | Protoplanetary disks | Constraint modelling | Radiative transfer | Modelling | Solar system | Interferometry | Collapse | Pollution sources | Density distribution | Rotation | Molecular chains | Emissions | Gas density | Organic chemistry | Dust | Morphology | Radio telescopes | Disks | Three dimensional models | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | Astronomi, astrofysik och kosmologi | ism | individual | molecules | formation | stars | iras 16293 | protostars | Astronomy, Astrophysics and Cosmology
Stars: protostars | Astrochemistry | Submillimeter: ISM | ISM: molecules | Stars: formation | ISM: individual objects: IRAS 16293-2422 (except planetary nebulae) | ORGANIC-MOLECULES | stars: protostars | HOT CORE | STAR-FORMATION | ROTATIONAL SPECTRUM | SUBMILLIMETER ARRAY | INTERSTELLAR-MEDIUM | OPHIUCHUS | LOW-MASS PROTOSTARS | stars: formation | YOUNG | submillimeter: ISM | ASTRONOMY & ASTROPHYSICS | IRAS-16293-2422 | astrochemistry | Angular resolution | Temperature regions | One dimensional models | Radiation | Luminosity | Emission | Protoplanetary disk | Density | Protostars | Protoplanetary disks | Constraint modelling | Radiative transfer | Modelling | Solar system | Interferometry | Collapse | Pollution sources | Density distribution | Rotation | Molecular chains | Emissions | Gas density | Organic chemistry | Dust | Morphology | Radio telescopes | Disks | Three dimensional models | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | Astronomi, astrofysik och kosmologi | ism | individual | molecules | formation | stars | iras 16293 | protostars | Astronomy, Astrophysics and Cosmology
Journal Article
Astronomy & astrophysics, ISSN 0004-6361, 01/2012, Volume 537, p. 17
Aims. In this paper the calibration and in-orbit performance of the Heterodyne Instrument for the Far-Infrared (HIFI) is described. Methods. The calibration of...
methods: observational | space vehicles: instruments | instrumentation: spectrographs | ASTRONOMY | ASTRONOMY & ASTROPHYSICS | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | astronomi | Astronomy | Astronomy, Astrophysics and Cosmology
methods: observational | space vehicles: instruments | instrumentation: spectrographs | ASTRONOMY | ASTRONOMY & ASTROPHYSICS | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | astronomi | Astronomy | Astronomy, Astrophysics and Cosmology
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2017, Volume 597, p. A53
Context. One of the open questions in astrochemistry is how complex organic and prebiotic molecules are formed. The unsurpassed sensitivity of the Atacama...
Astrochemistry | ISM: Individual object: IRAS 16293-2422 line: Identification | ISM: Abundances | Astrobiology | ISM: Molecules | ORION-KL | ORGANIC-MOLECULES | ISM: abundances | HOT CORE | COLOGNE DATABASE | MICROWAVE-SPECTRUM | STAR-FORMING REGIONS | INTERSTELLAR ACETONE | ISM: individual object: IRAS 16293-2422 line: identification | astrobiology | ISM: molecules | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | MOLECULAR-SPECTROSCOPY | LINE SURVEY | astrochemistry | Radio telescopes | Abundance | Mathematical models | Ethylene oxide | Excitation | Density | Protostars | Acetone | Other Chemical Engineering | Annan kemiteknik
Astrochemistry | ISM: Individual object: IRAS 16293-2422 line: Identification | ISM: Abundances | Astrobiology | ISM: Molecules | ORION-KL | ORGANIC-MOLECULES | ISM: abundances | HOT CORE | COLOGNE DATABASE | MICROWAVE-SPECTRUM | STAR-FORMING REGIONS | INTERSTELLAR ACETONE | ISM: individual object: IRAS 16293-2422 line: identification | astrobiology | ISM: molecules | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | MOLECULAR-SPECTROSCOPY | LINE SURVEY | astrochemistry | Radio telescopes | Abundance | Mathematical models | Ethylene oxide | Excitation | Density | Protostars | Acetone | Other Chemical Engineering | Annan kemiteknik
Journal Article
Astronomy & Astrophysics, ISSN 1432-0746, 2019, Volume 622, pp. 1 - 21
The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120-168 MHz survey of the entire northern sky for which observations are now...
Surveys | Techniques: image processing | Catalogs | Radio continuum: general | CALIBRATION | CLUSTER ENVIRONMENTS | surveys | radio continuum: general | AGN | UNDERSTANDING RADIO POLARIMETRY | IMAGING SURVEY | DISCOVERY | GALAXY | techniques: image processing | catalogs | ASTRONOMY & ASTROPHYSICS | SOUTHERN SKY | EMISSION | FLUX-DENSITY SCALE
Surveys | Techniques: image processing | Catalogs | Radio continuum: general | CALIBRATION | CLUSTER ENVIRONMENTS | surveys | radio continuum: general | AGN | UNDERSTANDING RADIO POLARIMETRY | IMAGING SURVEY | DISCOVERY | GALAXY | techniques: image processing | catalogs | ASTRONOMY & ASTROPHYSICS | SOUTHERN SKY | EMISSION | FLUX-DENSITY SCALE
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2018, Volume 610, p. A54
Context. The enhanced degrees of deuterium fractionation observed in envelopes around protostars demonstrate the importance of chemistry at low temperatures,...
ISM: individual objects: IRAS 16293-2422 | Stars: protostars | Astrochemistry | ISM: molecules | Stars: formation | STATE ROTATIONAL SPECTRUM | stars: protostars | GROUND-STATE | PREBIOTIC MOLECULE | COLOGNE DATABASE | INTERSTELLAR-MEDIUM | LOW-MASS PROTOSTARS | GRAIN-SURFACE-CHEMISTRY | stars: formation | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | MOLECULAR-SPECTROSCOPY | PHASE FORMATION | astrochemistry | Deuterium | Fractionation | Temperature | Energy levels | Formaldehyde | Thermodynamic equilibrium | Molecular chains | Protostars | Ice formation | Time dependence | Organic chemistry | Star formation | Spectral resolution | Radio telescopes | Excitation | Deuteration | Low temperature | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | Astronomi, astrofysik och kosmologi | Other Physics Topics | Atom- och molekylfysik och optik | Annan fysik | Atom and Molecular Physics and Optics | Astronomy, Astrophysics and Cosmology
ISM: individual objects: IRAS 16293-2422 | Stars: protostars | Astrochemistry | ISM: molecules | Stars: formation | STATE ROTATIONAL SPECTRUM | stars: protostars | GROUND-STATE | PREBIOTIC MOLECULE | COLOGNE DATABASE | INTERSTELLAR-MEDIUM | LOW-MASS PROTOSTARS | GRAIN-SURFACE-CHEMISTRY | stars: formation | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE PROTOSTAR | MOLECULAR-SPECTROSCOPY | PHASE FORMATION | astrochemistry | Deuterium | Fractionation | Temperature | Energy levels | Formaldehyde | Thermodynamic equilibrium | Molecular chains | Protostars | Ice formation | Time dependence | Organic chemistry | Star formation | Spectral resolution | Radio telescopes | Excitation | Deuteration | Low temperature | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | Astronomi, astrofysik och kosmologi | Other Physics Topics | Atom- och molekylfysik och optik | Annan fysik | Atom and Molecular Physics and Optics | Astronomy, Astrophysics and Cosmology
Journal Article