Search Results - "Miettinen, Oskari"
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A 3 mm Spectral Line Study of the Central Molecular Zone Infrared Dark Cloud G1.75-0.08
Published in Galaxies (01-08-2024)“…Infrared dark clouds (IRDCs) are fruitful objects to study the fragmentation of interstellar filaments and initial conditions and early stages of high-mass…”
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Dense cores in the Seahorse infrared dark cloud: physical properties from modified blackbody fits to the far-infrared-submillimetre spectral energy distributions
Published 09-11-2020“…We used data from WISE, IRAS, and Herschel in conjuction with our previous observations with SABOCA and LABOCA, and constructed the far-IR to submillimetre…”
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WISE J044232.92+322734.9: A star-forming galaxy at redshift 1.1 seen through a Galactic dust clump?
Published 02-10-2020“…Physically unassociated background or foreground objects seen towards submillimetre sources are potential contaminants of both the studies of young stellar…”
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What did the seahorse swallow? APEX 170 GHz observations of the chemical conditions in the Seahorse infrared dark cloud
Published 17-05-2020“…A&A 639, A65 (2020) We used the APEX telescope to observe spectral lines occurring at about 170 GHz frequency towards 14 positions along the full extent of the…”
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APEX observations of ortho-H$_2$D$^+$ towards dense cores in the Orion B9 filament
Published 13-01-2020“…A&A 634, A115 (2020) We used the APEX telescope to observe the 372 GHz o-H$_2$D$^+(J_{K_a,\,K_c}=1_{1,\,0}-1_{1,\,1})$ line towards three prestellar cores and…”
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A 3 mm spectral line study of the Central Molecular Zone infrared dark cloud G1.75-0.08
Published 26-06-2024“…Galaxies 2024, 12(4), 32 Infrared dark clouds (IRDCs) are fruitful objects to study the fragmentation of interstellar filaments and initial conditions and…”
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Protostellar classification using supervised machine learning algorithms
Published 25-08-2018“…Classification of young stellar objects (YSOs) into different evolutionary stages helps us to understand the formation process of new stars and planetary…”
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The Seahorse Nebula: New views of the filamentary infrared dark cloud G304.74+01.32 from SABOCA, Herschel, and WISE
Published 21-10-2017“…A&A 609, A123 (2018) We mapped the filamentary infrared dark cloud (IRDC) G304.74+01.32 at 350 $\mu$m with the SABOCA bolometer. The new SABOCA data have a…”
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ArT\'eMiS imaging of the filamentary infrared dark clouds G1.75-0.08 and G11.36+0.80: Dust-based physical properties of the clouds and their clumps
Published 09-09-2022“…A&A 667, A90 (2022) We imaged the infrared dark clouds (IRDCs) G1.75-0.08 and G11.36+0.80 at 350 $\mu$m and 450 $\mu$m using the ArT\'eMiS bolometer. These…”
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Characterising the physical and chemical properties of a young Class 0 protostellar core embedded in the Orion B9 filament
Published 27-06-2016“…The present study aims to characterise the physical and chemical properties of the protostellar core Orion B9-SMM3. The APEX telescope was used to perform a…”
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A MALT90 study of the chemical properties of massive clumps and filaments of infrared dark clouds
Published 18-11-2013“…We attempt to characterise the chemical properties of a sample of massive clumps of IRDCs through multi-molecular line observations. We also search for…”
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13CO and C18O J=2-1 mapping of the environment of the Class 0 protostellar core SMM 3 in Orion B9
Published 03-08-2012“…We attempt to achieve a better understanding of the gas distribution and velocity field around the deeply embedded Class 0 protostar SMM 3 in the Orion B9…”
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LABOCA 870 micron dust continuum mapping of selected infrared-dark cloud regions in the Galactic plane
Published 10-04-2012“…We have mapped four selected about 0.5 deg x 0.5 deg-sized fields containing Spitzer 8-micron dark regions with APEX/LABOCA at 870 micron. Selected positions…”
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A molecular line study of the filamentary infrared dark cloud G304.74+01.32
Published 14-02-2012“…The aim of this study is to better understand the physical and chemical properties of the filamentary IRDC G304.74+01.32. In particular, we aim to investigate…”
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LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32
Published 19-03-2010“…Infrared dark clouds (IRDCs) likely represent very early stages of high-mass star/star cluster formation. In this study, we aim to determine the physical…”
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On the Kennicutt-Schmidt scaling law of submillimetre galaxies
Published 02-06-2017“…The star formation rate per unit area correlates well with the gas surface density for different types of galaxies. However, this Kennicutt-Schmidt law has not…”
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Deuterium fractionation and the degree of ionisation in massive clumps within infrared dark clouds
Published 29-08-2011“…(Abridged) We aim to determine the degrees of CO depletion, deuterium fractionation, and ionisation in a sample of seven massive clumps associated with IRDCs…”
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Dynamics, CO depletion, and deuterium fractionation of the dense condensations within the fragmented prestellar core Orion B9-SMM 6
Published 10-05-2013“…We present APEX observations of C17O(2-1), N2H+(3-2), and N2D+(3-2) towards the subfragments inside the prestellar core SMM 6 in Orion B9. We combined these…”
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SABOCA 350-micron and LABOCA 870-micron dust continuum imaging of IRAS 05399-0121: mapping the dust properties of a pre- and protostellar core system
Published 05-04-2013“…We present a 350 micron APEX/SABOCA map of IRAS 05399-0121/SMM 1, which is a dense double-core system in Orion B9. We combined these data with our previous…”
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A (sub)millimetre study of dense cores in Orion B9
Published 21-12-2011“…We aim to further constrain the properties and evolutionary stages of dense cores in Orion B9. The central part of Orion B9 was mapped at 350 micron with…”
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