HGBS J041807.8+280506 , the SIMBAD biblio

HGBS J041807.8+280506 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.03.30CEST06:44:10


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Title First 3 Authors
2002ApJ...575..950O 145 126 A complete search for dense cloud cores in Taurus. ONISHI T., MIZUNO A., KAWAMURA A., et al.
2013A&A...554A..55H viz 18       D               3 33 159 Cores, filaments, and bundles: hierarchical core formation in the L1495/B213 Taurus region. HACAR A., TAFALLA M., KAUFFMANN J., et al.
2014MNRAS.439.3683M 175       D       C F     4 28 21 Properties of starless and prestellar cores in Taurus revealed by Herschel SPIRE/PACS imaging. MARSH K.A., GRIFFIN M.J., PALMEIRIM P., et al.
2016MNRAS.459..342M viz 16       D               1 550 31 A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey. MARSH K.A., KIRK J.M., ANDRE P., et al.
2016MNRAS.463.1008W viz 16       D               1 230 15 The JCMT and Herschel Gould Belt Surveys: a comparison of SCUBA-2 and Herschel data of dense cores in the Taurus dark cloud L1495. WARD-THOMPSON D., PATTLE K., KIRK J.M., et al.
2018A&A...617A..27P viz 27 ~ Kinematics of dense gas in the L1495 filament. PUNANOVA A., CASELLI P., PINEDA J.E., et al.
2021A&A...648A.120R 63       D     X         2 61 ~ Gas phase Elemental abundances in Molecular cloudS (GEMS). IV. Observational results and statistical trends. RODRIGUEZ-BARAS M., FUENTE A., RIVIERE-MARICHALAR P., et al.
2022A&A...657A..10S 1138       D S   X C       23 19 ~ Gas phase Elemental abundances in Molecular cloudS (GEMS) V. Methanol in Taurus. SPEZZANO S., FUENTE A., CASELLI P., et al.
2022ApJ...927..213P 19       D               1 29 ~ Methanol Mapping in Cold Cores: Testing Model Predictions. PUNANOVA A., VASYUNIN A., CASELLI P., et al.
2022A&A...662A..52E 65       D     X         2 61 ~ Gas phase Elemental abundances in Molecular cloudS (GEMS). VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission. ESPLUGUES G., FUENTE A., NAVARRO-ALMAIDA D., et al.

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2023.03.30-06:44:10

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