我没有强迫
发表于 2025-3-28 15:57:17
D. Rouan,D. Tiphène,F. Lacombe,P. Normandsverfahren.Ermöglicht Verständnis von schweren und systematiDas Buch arbeitet das Länderberichtsverfahren im interamerikanischen Menschenrechtsschutzsystem auf und liefert die erste umfassende und systematisierte Analyse des Länderberichtverfahrens der Interamerikanischen Kommission für Menschenrech
perjury
发表于 2025-3-28 19:00:55
Embedded Clusters: Problems but ProgressWe describe current problems and progress in the study of dense clusters of young stars embedded in the molecular clouds from which they recently formed.
GRATE
发表于 2025-3-29 00:00:34
Low-Luminosity Members of the R Coronae Australis Infrared ClusterPreliminary analysis is presented for J, H, and K′ images of the Corona Australis cloud core. Color-color and color-magnitude diagrams reveal relatively few new cluster members. We conclude that the R Cr A infrared cluster consists of only about 30 members and its size reflects the available reservoir of molecular gas.
cringe
发表于 2025-3-29 04:15:56
A New Wide-Field Infrared Survey Using Iris on the AATWe have completed observations for a new wide-field infrared survey. The survey covers a total area of 0.8 square degrees to a 5. limiting magnitude of ~ 17.5 at K′ (2.1 .m) and ~ 18.5 at H (1.6 .m). We present preliininary results from this survey, including galaxy colours and luminosities.
散开
发表于 2025-3-29 11:10:25
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显微镜
发表于 2025-3-29 14:41:44
Artillery Shells in OrionNear-infrared imaging of the Orion Molecular Cloud has revealed that an explosive event occurred in its core within the past 1000 years, ejecting at least a score of dense knots of gas at several 100 km/s.
Antagonism
发表于 2025-3-29 19:00:58
Photodissociation Regions in Young PNInfrared imaging of H2 and PAH emission in NGG 7027 and BD+30 3639 reveals the presence of photodissociation regions in the neutral gas surrounding these young planetary nebulae.
Cholecystokinin
发表于 2025-3-29 21:05:33
Spectra of a Remarkable Class of Hot Stars in the Galactic CenterTwo-micron spectra of several helium line stars in the galactic center have been obtained at UKIRT with CGS4. Lines studied include He I 2.058.m, He I 2.113.m, Br.2.166.m, and Pa.1.875.m. He/H in four of the stars is shown to be very overabundant.
终止
发表于 2025-3-30 02:41:38
https://doi.org/10.1007/978-94-011-1070-9Excel; Observatories; Redshift; astronomy; cosmology; imaging; instruments; spectroscopy
GOAT
发表于 2025-3-30 04:06:59
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