LDN 1375 , the SIMBAD biblio

LDN 1375 , the SIMBAD biblio (13 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:39:43


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Title First 3 Authors
1962ApJS....7....1L viz 1829 890 Catalogue of dark nebulae. LYNDS B.T.
1973ApJ...183..449D 420 95 A survey of interstellar formaldehyde in dust clouds. DIETER N.H.
1988IRASP.C......0J viz 14       D               1 245223 ~ Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 JOINT IRAS SCIENCE WORKING GROUP
1991A&A...248..209T 87 41 An OH survey of very cold IRAS point sources. TE LINTEL HEKKERT P.
1996A&AS..115...81B viz 1472 529 A CS(2-1) survey of IRAS point sources with color characteristics of ultra-compact HII regions. BRONFMAN L., NYMAN L.-A. and MAY J.
2002ApJ...578..229S 59 33 Molecular clouds and stellar clusters in the far outer galaxy. SNELL R.L., CARPENTER J.M. and HEYER M.H.
2003A&A...399.1083K viz 6713 27 The association of IRAS sources and 12CO emission in the outer Galaxy. KERTON C.R. and BRUNT C.M.
2003ApJ...595..900K 70 42 Triggered star formation in the W5 H II region. KARR J.L. and MARTIN P.G.
2007PASJ...59.1185S viz 15       D               1597 41 Water maser and ammonia survey toward IRAS sources in the Galaxy. I. H2O maser data. SUNADA K., NAKAZATO T., IKEDA N., et al.
2009A&A...507..369W 15       D               1 106 17 The relation between 13CO J = 2-1 line width in molecular clouds and bolometric luminosity of associated IRAS sources. WANG K., WU Y.F., RAN L., et al.
2011MNRAS.418.2121G viz 76           X         2 130 22 JCMT HARP CO 3–2 observations of molecular outflows in W5. GINSBURG A., BALLY J. and WILLIAMS J.P.
2017AJ....154..163I viz 373       D     X C       9 19 2 Star formation activity beyond the Outer Arm. I. WISE-selected candidate star-forming regions. IZUMI N., KOBAYASHI N., YASUI C., et al.
2024MNRAS.527.8151S 108       D         F     13 31 ~ An improved method to measure 12C/13C and 14N/15N abundance ratios: revisiting CN isotopologues in the Galactic outer disc. SUN Y., ZHANG Z.-Y., WANG J., et al.

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