2003, 1 Auflage., Entwicklungsperspektiven, ISBN 3899585194, Volume 80
Book
Astronomy and Astrophysics, ISSN 0004-6361, 05/2018, Volume 613, p. L6
Debris disks are usually detected through the infrared excess over the photospheric level of their host star. The most favorable stars for disk detection are...
Protoplanetary disks | Techniques: high angular resolution | Stars: individual: GSC 07396-00759 | DUST | PROFILES | stars: individual: GSC 07396-00759 | DEBRIS DISKS | SEARCH | ASTRONOMY & ASTROPHYSICS | MASS | techniques: high angular resolution | protoplanetary disks | SPECTRA | Stellar winds | Terrestrial planets | Image resolution | Space debris | Asymmetric structures | Terrestrial environments | Detritus | M stars | Accretion disks | Inclination | Red dwarf stars | Photosphere | Planets | Planet detection | Binary stars | Companion stars | Debris | Deposition | Image contrast | Physics - Earth and Planetary Astrophysics | Physics | Astrophysics | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Protoplanetary disks | Techniques: high angular resolution | Stars: individual: GSC 07396-00759 | DUST | PROFILES | stars: individual: GSC 07396-00759 | DEBRIS DISKS | SEARCH | ASTRONOMY & ASTROPHYSICS | MASS | techniques: high angular resolution | protoplanetary disks | SPECTRA | Stellar winds | Terrestrial planets | Image resolution | Space debris | Asymmetric structures | Terrestrial environments | Detritus | M stars | Accretion disks | Inclination | Red dwarf stars | Photosphere | Planets | Planet detection | Binary stars | Companion stars | Debris | Deposition | Image contrast | Physics - Earth and Planetary Astrophysics | Physics | Astrophysics | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2018, Volume 618, p. A23
A&A 618, A23 (2018) Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less...
Techniques: high angular resolution | Stars: pre-main sequence | Binaries: visual | Stars: individual: GJ 2060 | Stars: low-mass | Stars: individual: TWA 22 | Astrometry
Techniques: high angular resolution | Stars: pre-main sequence | Binaries: visual | Stars: individual: GJ 2060 | Stars: low-mass | Stars: individual: TWA 22 | Astrometry
Journal Article
Atherosclerosis, ISSN 0021-9150, 08/2018, Volume 275, pp. 304 - 311
Plasma apolipoprotein M (APOM) is bound to HDL-particles and has anti-atherogenic effects. The present study explored whether plasma APOM is reduced in...
LDL-cholesterol | Urine apolipoprotein M sphingosine-1-phosphate | Chronic kidney disease | Plasma apolipoprotein M | Cardiovascular risk | HDL cholesterol | CARDIAC & CARDIOVASCULAR SYSTEMS | BETA-HDL FORMATION | RECEPTOR | ATHEROSCLEROSIS RISK | ARTERIAL-DISEASE | APOM CONFER | INSULIN-RESISTANCE | PROMOTER REGION | PERIPHERAL VASCULAR DISEASE | CORONARY-HEART-DISEASE | STAGE RENAL-DISEASE | Care and treatment | Chronic kidney failure | Blood cholesterol | Low density lipoproteins | Sphingosine | Liquid chromatography | Apolipoproteins
LDL-cholesterol | Urine apolipoprotein M sphingosine-1-phosphate | Chronic kidney disease | Plasma apolipoprotein M | Cardiovascular risk | HDL cholesterol | CARDIAC & CARDIOVASCULAR SYSTEMS | BETA-HDL FORMATION | RECEPTOR | ATHEROSCLEROSIS RISK | ARTERIAL-DISEASE | APOM CONFER | INSULIN-RESISTANCE | PROMOTER REGION | PERIPHERAL VASCULAR DISEASE | CORONARY-HEART-DISEASE | STAGE RENAL-DISEASE | Care and treatment | Chronic kidney failure | Blood cholesterol | Low density lipoproteins | Sphingosine | Liquid chromatography | Apolipoproteins
Journal Article
Astronomy and Astrophysics - A&A, ISSN 0004-6361, 2018, Volume 618, p. A23
Context. Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less reliable at...
Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article
THYROID, ISSN 1050-7256, 09/2016, Volume 26, Issue 9, pp. 1149 - 1153
Journal Article
The New England Journal of Medicine, ISSN 0028-4793, 12/2005, Volume 353, Issue 24, pp. 2550 - 2558
This double-blind, randomized, noninferiority trial prospectively evaluated the effect of oral contraceptives on lupus activity in premenopausal women with...
UNITED-STATES | TRIAL | MEDICINE, GENERAL & INTERNAL | THERAPY | FREQUENCY | ESTROGEN | CLASSIFICATION | RISK | SLE | OSTEOPOROSIS | DISEASE-ACTIVITY | Pregnancy | Severity of Illness Index | Ethinyl Estradiol - adverse effects | Double-Blind Method | Humans | Norethindrone - adverse effects | Adolescent | Lupus Erythematosus, Systemic - classification | Adult | Female | Contraceptives, Oral, Combined - adverse effects | Women | Usage | Systemic lupus erythematosus | Oral contraceptives | Health aspects | Menopause | Lupus | Birth control | Autoimmune diseases | Womens health
UNITED-STATES | TRIAL | MEDICINE, GENERAL & INTERNAL | THERAPY | FREQUENCY | ESTROGEN | CLASSIFICATION | RISK | SLE | OSTEOPOROSIS | DISEASE-ACTIVITY | Pregnancy | Severity of Illness Index | Ethinyl Estradiol - adverse effects | Double-Blind Method | Humans | Norethindrone - adverse effects | Adolescent | Lupus Erythematosus, Systemic - classification | Adult | Female | Contraceptives, Oral, Combined - adverse effects | Women | Usage | Systemic lupus erythematosus | Oral contraceptives | Health aspects | Menopause | Lupus | Birth control | Autoimmune diseases | Womens health
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 10/2018, Volume 618
Context. Evolutionary models are widely used to infer the mass of stars, brown dwarfs, and giant planets. Their predictions are thought to be less reliable at...
EXTRASOLAR PLANETS | AB-DORADUS-C | LITHIUM DEPLETION | binaries: visual | stars: individual: GJ 2060 | BETA-PICTORIS | stars: individual: TWA22 | BROWN DWARF | stars: pre-main sequence | AO SYSTEM | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | techniques: high angular resolution | STARS | stars: low-mass | TW-HYDRAE ASSOCIATION | astrometry | HR 8799 | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
EXTRASOLAR PLANETS | AB-DORADUS-C | LITHIUM DEPLETION | binaries: visual | stars: individual: GJ 2060 | BETA-PICTORIS | stars: individual: TWA22 | BROWN DWARF | stars: pre-main sequence | AO SYSTEM | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | techniques: high angular resolution | STARS | stars: low-mass | TW-HYDRAE ASSOCIATION | astrometry | HR 8799 | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2018, Volume 617, p. L2
A&A 617, L2 (2018) Aims: We aim to characterize the orbital and atmospheric properties of PDS 70 b, which was first identified on May 2015 in the course of the...
Methods: observational | Planets and satellites: atmospheres | Planets and satellites: individual: PDS 70 | Techniques: spectroscopic | Astrometry | Physics - Earth and Planetary Astrophysics | Earth and Planetary Astrophysics | Sciences of the Universe | Astrophysics
Methods: observational | Planets and satellites: atmospheres | Planets and satellites: individual: PDS 70 | Techniques: spectroscopic | Astrometry | Physics - Earth and Planetary Astrophysics | Earth and Planetary Astrophysics | Sciences of the Universe | Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2018, Volume 617, p. A44
Context. Young circumstellar disks are the birthplaces of planets. Their study is of prime interest to understand the physical and chemical conditions under...
Stars: individual: PDS 70 | Techniques: high angular resolution | Radiative transfer | Planets and satellites: detection | Protoplanetary disks | Scattering | stars: individual: PDS 70 | radiative transfer | GIANT PLANETS | CANDIDATE | GRAINS | scattering | BROWN DWARFS | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | YOUNG STAR | techniques: high angular resolution | protoplanetary disks | T-TAURI STARS | planets and satellites: detection | Planetary atmospheres | Rayleigh scattering | Extrasolar planets | Atmospheric models | Luminosity | Spatial analysis | Planetary mass | Infrared analysis | Infrared imagery | Accretion disks | Image detection | Astrometry | Organic chemistry | Planets | Wavelengths | Planet detection | Protoplanets | Planet formation | Planetary evolution | Infrared imaging | Evolution | Polarimetry | Brightness distribution | Physics - Earth and Planetary Astrophysics | Sciences of the Universe | Astrophysics | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Stars: individual: PDS 70 | Techniques: high angular resolution | Radiative transfer | Planets and satellites: detection | Protoplanetary disks | Scattering | stars: individual: PDS 70 | radiative transfer | GIANT PLANETS | CANDIDATE | GRAINS | scattering | BROWN DWARFS | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | YOUNG STAR | techniques: high angular resolution | protoplanetary disks | T-TAURI STARS | planets and satellites: detection | Planetary atmospheres | Rayleigh scattering | Extrasolar planets | Atmospheric models | Luminosity | Spatial analysis | Planetary mass | Infrared analysis | Infrared imagery | Accretion disks | Image detection | Astrometry | Organic chemistry | Planets | Wavelengths | Planet detection | Protoplanets | Planet formation | Planetary evolution | Infrared imaging | Evolution | Polarimetry | Brightness distribution | Physics - Earth and Planetary Astrophysics | Sciences of the Universe | Astrophysics | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A57
Context. 51 Eridani b is an exoplanet around a young (20 Myr) nearby (29.4 pc) F0-type star, which was recently discovered by direct imaging. It is one of the...
Techniques: high angular resolution | Planets and satellites: atmospheres | Techniques: image processing | Stars: individual: 51 Eridani | Methods: data analysis | planets and satellites: atmospheres | PHYSICAL-PROPERTIES | methods: data analysis | DIRECTLY IMAGED EXOPLANET | HR 8799 PLANETS | T-DWARFS | stars: individual: 51 Eridani | FINDER SPHERE II | OPTICAL-TRANSMISSION SPECTRUM | VERY-LOW-MASS | techniques: image processing | BROWN DWARFS | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | techniques: high angular resolution | 1ST LIGHT | Analytical methods | Clouds | Atmospheric models | Luminosity | Optics | Spectroscopic analysis | Iron | Conditional probability | Adaptive control | Brown dwarf stars | Imaging | Masking | Solar system | Detection limits | Photometry | Gravitation | Parameters | Architecture | Extrasolar planets | Spectra | Adaptive search techniques | Sedimentation | Cold starts | Cloud cover | Planets | Spectrographs | Metallicity | Integrals | Very Large Telescope | Adaptive optics | Spectrophotometry | Physics - Earth and Planetary Astrophysics | Sciences of the Universe | Physics | Astrophysics | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
Techniques: high angular resolution | Planets and satellites: atmospheres | Techniques: image processing | Stars: individual: 51 Eridani | Methods: data analysis | planets and satellites: atmospheres | PHYSICAL-PROPERTIES | methods: data analysis | DIRECTLY IMAGED EXOPLANET | HR 8799 PLANETS | T-DWARFS | stars: individual: 51 Eridani | FINDER SPHERE II | OPTICAL-TRANSMISSION SPECTRUM | VERY-LOW-MASS | techniques: image processing | BROWN DWARFS | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | techniques: high angular resolution | 1ST LIGHT | Analytical methods | Clouds | Atmospheric models | Luminosity | Optics | Spectroscopic analysis | Iron | Conditional probability | Adaptive control | Brown dwarf stars | Imaging | Masking | Solar system | Detection limits | Photometry | Gravitation | Parameters | Architecture | Extrasolar planets | Spectra | Adaptive search techniques | Sedimentation | Cold starts | Cloud cover | Planets | Spectrographs | Metallicity | Integrals | Very Large Telescope | Adaptive optics | Spectrophotometry | Physics - Earth and Planetary Astrophysics | Sciences of the Universe | Physics | Astrophysics | Fysik | Physical Sciences | Astronomi, astrofysik och kosmologi | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2017, Volume 605, p. L9
\ Aims. The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars aimed at searching for and characterizing new planetary systems...
Instrumentation: adaptive optics | Methods: observational | Planets and satellites: atmospheres | Instrumentation: high angular resolution | Planets and satellites: formation | instrumentation: adaptive optics | planets and satellites: atmospheres | methods: observational | YOUNG | SPECTROSCOPY | BROWN DWARFS | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | STARS | instrumentation: high angular resolution | planets and satellites: formation | COMPANION | Clouds | Atmospheric models | Luminosity | Stellar coronas | Image acquisition | Planet detection | Planet formation | Infrared imaging | Evolution | Photometry | Image contrast | Effective temperatures | Gravitation | Test procedures | Infrared spectra | Infrared signatures | Infrared imagery | Near infrared radiation | Organic chemistry | Population (statistical) | Jupiter | Planets | Planetary evolution | Atmosphere | Stellar age | Planetary systems | Sciences of the Universe | Astrophysics | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Instrumentation: adaptive optics | Methods: observational | Planets and satellites: atmospheres | Instrumentation: high angular resolution | Planets and satellites: formation | instrumentation: adaptive optics | planets and satellites: atmospheres | methods: observational | YOUNG | SPECTROSCOPY | BROWN DWARFS | ASTRONOMY & ASTROPHYSICS | EVOLUTIONARY MODELS | STARS | instrumentation: high angular resolution | planets and satellites: formation | COMPANION | Clouds | Atmospheric models | Luminosity | Stellar coronas | Image acquisition | Planet detection | Planet formation | Infrared imaging | Evolution | Photometry | Image contrast | Effective temperatures | Gravitation | Test procedures | Infrared spectra | Infrared signatures | Infrared imagery | Near infrared radiation | Organic chemistry | Population (statistical) | Jupiter | Planets | Planetary evolution | Atmosphere | Stellar age | Planetary systems | Sciences of the Universe | Astrophysics | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
Journal Article