1,725,731 research outputs found

    Santa Fe (ATSF) 4029

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    A photograph print showing Santa Fe (ATSF) 4029, 2-8-2, So. Shawnee, OK

    Block Card 4029 Marlaine Drive

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    This 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 | Ranch houses | Talmadge Estates (Toledo, Ohio) | Westgate Area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | 4029 Marlaine Drive (Toledo, Ohio

    Telegram re: S. 4029

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    Telegram from Amon G. Carter to Lyndon B. Johnson re: the passage of S. 4029 by the House and his urgence to Johnson to convince others of the need to pass the amendments specifically relevant to osteopathy. Also included is the telegram confirmation and rough draf

    Block Card 4029 Deepwood Lane

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    This 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: Split-Level Style | 4029 Deepwood Lane (Toledo, Ohio) | Dwelling | Copland Heights (Toledo, Ohio) | South Toledo Area (Toledo, Ohio

    Block Card 4029 Crary Drive

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    This 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 | 4029 Crary Drive (Toledo, Ohio) | Ranch houses | Delrea Place (Toledo, Ohio) | Deveaux Area (Toledo, Ohio) | West Toledo area (Toledo, Ohio

    Block Card 4029 Arnelle Road

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    This 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 – Ohio – Toledo | Ranch Style | Meadowland Estates (Toledo, Ohio) | Westgate Area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | 4029 Arnelle Road (Toledo, Ohio

    AFGL 4029: a cluster of massive young stars

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    International audienceThe molecular cloud IC 1848A, located at the border of the extended H ii region S 199, harbors the bright in-frared source AFGL 4029. A young star cluster is observed in this direction. We present an optical and near infrared study of this cluster, which contains at least thirty B stars. The visual extinction affecting the stars attains 30 mag, and shows large variations on very small scales. The most massive star, possibly a B1V, ionizes the ultracompact H ii region G138.300+1.558. The youngest object of the cluster, AFGL 4029-IRS 1-identical to the radio source G138.295+1.555-is a massive pre-main-sequence object illuminating a reflection nebula. AFGL 4029-IRS 1 is luminous (∼ 10 4 L) and highly reddened (A V = 25-30 mag); displaying many of the spectral characteristics of pre-main-sequence objects (including bright and broad emission lines and the presence of Fe ii emission), it is very similar to the most luminous Herbig Ae/Be stars. AFGL 4029-IRS 1 shows evidence of mass ejection: it emits an ionized stellar wind with terminal velocities of about 400 km s −1 and a mass loss rate of about 7 10 −6 M yr −1 ; it is associated with a CO outflow and a high velocity optical jet; a bright unresolved H 2 clump is observed in its vicinity. The whole complex is a very efficient star forming region, as about 10% of the mass of the parental molecular cloud has been used to form B stars

    Data for: Multi-wavelength study in the region of IRAS 16571-4029 and 16575-4023 sources

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    Table 3: Catalog with astrometric and multiband photometric information for about 44600 objects in the region of IRAS 16571-4029 and 16575-4023 sources Table 4: Selected objects in the region of IRAS 16571-4029 source. Table 8: OB candidates in the region of IRAS 16575-4023 (B) sourc

    Linked collectors and determiners for: Phytoplankton community composition at station Svartnes, Balsfjord, Norway in June 2017 and June 2018 (sampled with a GoFlow bottle).

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    Natural history specimen data linked to collectors and determiners held within, "Phytoplankton community composition at station Svartnes, Balsfjord, Norway in June 2017 and June 2018 (sampled with a GoFlow bottle)". Claims or attributions were made on Bionomia by volunteer Scribes, <a href="http://bionomia.net/dataset/5e2eccfd-47a8-4029-946a-c1bec35d86b7">https://bionomia.net/dataset/5e2eccfd-47a8-4029-946a-c1bec35d86b7</a> using specimen data from the dataset aggregated by the Global Biodiversity Information Facility, <a href="https://gbif.org/dataset/5e2eccfd-47a8-4029-946a-c1bec35d86b7">https://gbif.org/dataset/5e2eccfd-47a8-4029-946a-c1bec35d86b7</a>. Formatted as a Frictionless Data package

    Data for: Multi-wavelength study in the region of IRAS 16571-4029 and 16575-4023 sources

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    Table 3: Catalog with astrometric and multiband photometric information for about 44600 objects in the region of IRAS 16571-4029 and 16575-4023 sourcesTable 4: Selected objects in the region of IRAS 16571-4029 source.Table 8: OB candidates in the region of IRAS 16575-4023 (B) sourc
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