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Reliability conditions of Eh measurements in lake sediments. EUR 6035 EN. Environment and quality of life
Full text linkBlock Card 6035 Atwell Road
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | 6035 Atwell Road (Toledo, Ohio) | Dwelling | Edgehill Subdivision (Toledo, Ohio) | Trilby Area (Toledo, Ohio)
Block Card 6035 Lewis Avenue
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | 6035 Lewis Avenue (Toledo, Ohio) | Dwelling | Greenwood Park Area (Toledo, Ohio
Block Card 6035 Pickard Drive
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Dwelling | 6035 Pickard Drive (Toledo, Ohio) | Hopewell Acres (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | West Toledo Area (Toledo, Ohio) | Folk House Styl
Block Card 6035 Jackman Road
No full textThis image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Dwelling | 6035 Jackman Road (Toledo, Ohio) | Side gabled | Hopewell Acres (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | West Toledo Area (Toledo, Ohio) | Folk House Styl
A search for the OH 6035 MHz line in high-mass star-forming regions
Full text linkContext. The excited states of OH masers detected in the environment of high-mass young stellar objects (HMYSOs) are important for improving our understanding of the physical conditions of these objects and also provide information about their magnetic fields.
Aims. We aim to search for excited-state OH 6035 MHz maser emission in HMYSOs which might have escaped detection in previous surveys or were never searched for.
Methods. A sample of HMYSOs derived from untargeted surveys of the 6668 MHz methanol maser line was observed at 6035 MHz OH transition with the Torun 32 m radio telescope. The 6035 MHz detections were observed in the OH 6031 MHz line. Two-thirds of the detections were observed at least three times over a two-year period.
Results. Out of 445 targets, 37 were detected at 6035 MHz, including seven new discoveries. The 6031 MHz line was detected towards ten 6035 MHz sources, one of which was not previously reported. All the newly detected sources are faint with the peak flux density lower than 4 Jy and show significant or high variability on timescales of 4 to 20 months. Zeeman pair candidates identified in three
new sources imply a magnetic field intensity of 2-11 mG. Comparison of our spectra with those obtained ~10 yr ago indicates different degrees of variability but there is a general increase in the variability index on an ~25 yr timescale, usually accompanied by significant changes in the profile shape.NCN 2016/21/B/ST9/0145
A search for the OH 6035 MHz line in high-mass star-forming regions
No full textContext. The excited states of OH masers detected in the environment of high-mass young stellar objects (HMYSOs) are important for improving our understanding of the physical conditions of these objects and also provide information about their magnetic fields.
Aims. We aim to search for excited-state OH 6035 MHz maser emission in HMYSOs which might have escaped detection in previous surveys or were never searched for.
Methods. A sample of HMYSOs derived from untargeted surveys of the 6668 MHz methanol maser line was observed at 6035 MHz OH transition with the Torun 32 m radio telescope. The 6035 MHz detections were observed in the OH 6031 MHz line. Two-thirds of the detections were observed at least three times over a two-year period.
Results. Out of 445 targets, 37 were detected at 6035 MHz, including seven new discoveries. The 6031 MHz line was detected towards ten 6035 MHz sources, one of which was not previously reported. All the newly detected sources are faint with the peak flux density lower than 4 Jy and show significant or high variability on timescales of 4 to 20 months. Zeeman pair candidates identified in three new sources imply a magnetic field intensity of 2–11 mG. Comparison of our spectra with those obtained ~10 yr ago indicates different degrees of variability but there is a general increase in the variability index on an ~25 yr timescale, usually accompanied by significant changes in the profile shape
Force theory for multiphase bodies
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Previous issue date: 1995-12DMS 92 95/12; DMS 92 06241 95/1
The strong/weak syllable distinction in English
Full text linkContains fulltext :
6035.pdf (Publisher’s version ) (Open Access
Il P. Michigan inv. 6035 dei Cavalieri di Aristofane (LDAB 351=CGFP 27)
No full textAim of this paper is to evaluate the importance of P. Michigan inv. 6035 in matter of
strophic articulation of the song. This papyrus shows a different system in comparison with what is known from heliodorean tradition
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