157 research outputs found
Hochauflösende Beobachtungen ultrakompakter HII-Gebiete
Die Arbeit präsentiert Ergebnisse von Breit- und Schmalbandbeobachtungen ultrakompakter HII-Gebiete im nahen und mittleren Infrarot. Erstmals kam im NIR ein System adaptiver Optik (ADONIS am 3.6m-Teleskop der ESO) umfassend fuer die Untersuchung dieser Objektklasse zum Einsatz. In der Arbeit werden zunaechst die bestehenden Modellvorstellungen zu ultrakompakten HII-Gebieten zusammengefasst. Dann wird die notwendigkeit hochaufloesender Infrarotbeobachtungen gezeigt sowie - als Loesungsansatz - die Methodik der adaptiven Optik umrissen. Praesentiert werden Ergebnisse zu den Objekten G45.45+0.06, G5.89-0.39 und G5.97-1.17. Darin werden der stellare Inhalt der genannten Gebiete sowie ihre Staubmassen und Ionisationsstrukturen charakterisiert. Hinsichtlich des Sternentstehungsprozesses bestaetigt sich, dass massereiche Sterne in Haufen entstehen. In G45 konnten dank der erreichten Aufloesung 8 Objekte als massereiche Sterne vom Spektraltyp O identifiziert und
somit nachgewiesen werden, daĂź zumindest einige ultrakompakte HII-Gebiete von Haufen ionisiert werden. Die ultrakompakten HII-Gebiete bilden sich in der Regel durch Verschmelzung individueller Ionisationszonen, oder sie gehen auf einzelne Haufenmitglieder zurueck. Warmer Staub ist in allen dr ei Gebieten vorhanden, in G45 ist die Emission dieses Staubes aus denselben Gebieten zu beobachten wie die Frei-frei-Strahlung des ionisierten Plasmas. Ob dies ein Projektionseffekt ist, bedarf noch der UeberprĂĽfung, auf jeden Fall ist in allen drei Gebi eten warmer Staub an der Grenzschicht zum ionisierten
Gas vorhanden. Die Materieverteilung bestimmt bei G45 und G5.89 auch die Morphologie. Bei einer Einordnung in bestehende Modellvorstellungen zu ultrakompakten HII-Gebieten wird entsprechend dargelgt, d aĂź auf dynamische Modelle kein Hinweis besteht sondern alleine die Staubmengen deren Verteilung zur Loesung des "Lebensdauerproblems" und der Erklaerung der Erscheinungsformen ausreichen
Frame Combination Techniques for Ultra High-Contrast Imaging
We summarize here an experimental frame combination pipeline we developed for
ultra high-contrast imaging with systems like the upcoming VLT SPHERE
instrument. The pipeline combines strategies from the Drizzle technique, the
Spitzer IRACproc package, and homegrown codes, to combine image sets that may
include a rotating field of view and arbitrary shifts between frames. The
pipeline is meant to be robust at dealing with data that may contain non-ideal
effects like sub-pixel pointing errors, missing data points, non-symmetrical
noise sources, arbitrary geometric distortions, and rapidly changing point
spread functions. We summarize in this document individual steps and
strategies, as well as results from preliminary tests and simulations.Comment: 9 pages, 4 figures, SPIE conference pape
Single conjugate adaptive optics for the ELT instrument METIS
The ELT is a 39m large, ground-based optical and near- to mid-infrared
telescope under construction in the Chilean Atacama desert. Operation is
planned to start around the middle of the next decade. All first light
instruments will come with wavefront sensing devices that allow control of the
ELT's intrinsic M4 and M5 wavefront correction units, thus building an adaptive
optics (AO) system. To take advantage of the ELT's optical performance, full
diffraction-limited operation is required and only a high performance AO system
can deliver this. Further technically challenging requirements for the AO come
from the exoplanet research field, where the task to resolve the very small
angular separations between host star and planet, has also to take into account
the high-contrast ratio between the two objects. We present in detail the
results of our simulations and their impact on high-contrast imaging in order
to find the optimal wavefront sensing device for the METIS instrument. METIS is
the mid-infrared imager and spectrograph for the ELT with specialised
high-contrast, coronagraphic imaging capabilities, whose performance strongly
depends on the AO residual wavefront errors. We examined the sky and target
sample coverage of a generic wavefront sensor in two spectral regimes, visible
and near-infrared, to pre-select the spectral range for the more detailed
wavefront sensor type analysis. We find that the near-infrared regime is the
most suitable for METIS. We then analysed the performance of Shack-Hartmann and
pyramid wavefront sensors under realistic conditions at the ELT, did a
balancing with our scientific requirements, and concluded that a pyramid
wavefront sensor is the best choice for METIS. For this choice we additionally
examined the impact of non-common path aberrations, of vibrations, and the
long-term stability of the SCAO system including high-contrast imaging
performance.Comment: 37 pages, 27 figures, accepted for publication in Experimental
Astronom
SPOTS: The Search for Planets Orbiting Two Stars. I. Survey description and first observations
Direct imaging surveys for exoplanets commonly exclude binary stars from
their target lists, leaving a large part of the overall planet demography
unexplored. To address this gap in our understanding of planet formation and
evolution, we have launched the first direct imaging survey dedicated to
circumbinary planets: SPOTS, the Search for Planets Orbiting Two Stars. In this
paper, we discuss the theoretical context, scientific merit, and technical
feasibility of such observations, describe the target sample and observational
strategy of our survey, and report on the first results from our pilot survey
of 26 targets with the VLT NaCo facility. While we have not found any confirmed
substellar companions to date, a number of promising candidate companions
remain to be tested for common proper motion in upcoming follow-up
observations. We also report on the astrometry of the three resolved binaries
in our target sample. This pilot survey constitutes a successful proof of
concept for our survey strategy and paves the way for a second stage of
exploratory observations with VLT SPHERE.Comment: 12 pages, 4 figures, 3 tables. Accepted for publication in A&
Infrared Observation of Hot Cores
We report on mid-infrared imaging of hot cores performed with SpectroCam-10
and TIMMI2. The observations aimed at the detection of thermal emission
presumably associated with the hot cores. Mid-infrared flux measurements are
required to improve the luminosity and optical depth estimates for these
sources. Results are presented for W3(HO), G9.62+0.19, G10.47+0.03, and the
possible hot core candidate G232.620+0.996. They illustrate that the morphology
of these sources cannot be described by simple geometries. Therefore,
line-of-sight effects and considerable extinction even at mid-infrared
wavelengths must not be neglected.Comment: 6 pages, 4 figures, Conference proceeding "Origins of stars and
planets: The VLT view", ESO, Garching, April 24-27 200
Simulating METIS SCAO System
METIS, the Mid-Infrared ELT Imager and Spectrograph, is one of the four
first-generation ELT instruments scheduled to see first light in 2028. Its two
main science modules are supported by an adaptive optics system featuring a
pyramid sensor with 90x90 subapertures working in the H and K bands. During the
PDR and FDR phases, extensive simulations were carried out to support the
sensing, reconstruction, and control concept of METIS single-conjugate adaptive
optics (SCAO) system. We present details on the implementation of the
COMPASS-based environment used for the simulations, the metrics used for
analyzing our performance expectations, an overview of the main results, and
some details on special cases like non-common path aberrations (NCPA) and water
vapor seeing, as well as the low-wind effect.Comment: 17 pages, 14 Figures, AO4ELT VII Conference - Avignon - June 202
The VLTI/MIDI survey of massive young stellar objects - Sounding the inner regions around intermediate- and high-mass young stars using mid-infrared interferometry
We aim to characterize the distribution and composition of circumstellar
material around young massive stars, and to investigate exactly which physical
structures in these objects are probed by long-baseline mid-infrared
interferometric observations. We used the two-telescope interferometric
instrument MIDI of the Very Large Telescope Interferometer of the European
Southern Observatory to observe a sample of 24 intermediate- and high-mass
young stellar objects in the N band (8-13 micron). We had successful fringe
detections for 20 objects, and present spectrally-resolved correlated fluxes
and visibility levels for projected baselines of up to 128 m. We fit the
visibilities with geometric models to derive the sizes of the emitting regions,
as well as the orientation and elongation of the circumstellar material.
Fourteen objects in the sample show the 10 micron silicate feature in
absorption in the total and correlated flux spectra. For 13 of these objects,
we were able to fit the correlated flux spectra with a simple absorption model,
allowing us to constrain the composition and absorptive properties of the
circumstellar material. Nearly all of the massive young stellar objects
observed show significant deviations from spherical symmetry at mid-infrared
wavelengths. In general, the mid-infrared emission can trace both disks and
outflows, and in many cases it may be difficult to disentangle these components
on the basis of interferometric data alone, because of the sparse spatial
frequency coverage normally provided by current long-baseline interferometers.
For the majority of the objects in this sample, the absorption occurs on
spatial scales larger than those probed by MIDI. Finally, the physical extent
of the mid-infrared emission around these sources is correlated with the total
luminosity, albeit with significant scatter.Comment: 36 pages, 22 figures. Accepted to Astronomy and Astrophysic
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