MSXDC G304.74+1.32 , the SIMBAD biblio

MSXDC G304.74+1.32 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:44:41

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2010A&A...520A.102M 1983 T   A D S   X C       50 54 21 LABOCA mapping of the infrared dark cloud
MSXDC

G304.74+01.32. 		MIETTINEN O. and HARJU J.
2012A&A...540A.104M 1996 T K A S   X C       49 27 21 A molecular line study of the filamentary infrared dark cloud

G304.74+01.32. 		MIETTINEN O.
2012A&A...542A.101M viz 116           X         3 164 15 LABOCA 870 µm dust continuum mapping of selected infrared-dark cloud regions in the Galactic plane. MIETTINEN O.
2012ApJ...756...10L 39           X         1 36 39 Fragmentation and OB star formation in high-mass molecular hub-filament systems. LIU H.B., JIMENEZ-SERRA I., HO P.T.P., et al.
2013ApJ...766...68P 117           X C       2 36 14 G048.66-0.29: physical state of an isolated site of massive star formation. PITANN J., LINZ H., RAGAN S., et al.
2013ApJ...766..115K 49           X         1 11 239 Filamentary accretion flows in the embedded Serpens South protocluster. KIRK H., MYERS P.C., BOURKE T.L., et al.
2018A&A...609A.123M viz 5622 T K A S   X C       134 23 2 The Seahorse Nebula: New views of the filamentary infrared dark cloud

G304.74+01.32 from SABOCA, Herschel, and WISE. 		MIETTINEN O.
2020A&A...639A..65M 366   K A     X C       8 20 ~ What did the seahorse swallow? APEX 170 GHz observations of the chemical conditions in the Seahorse infrared dark cloud. MIETTINEN O.
2020A&A...644A..82M 238   K A     X C       5 16 ~ Dense cores in the Seahorse infrared dark cloud: physical properties from modified blackbody fits to the far-infrared-submillimetre spectral energy distributions. MIETTINEN O.
2022A&A...667A..90M 45           X         1 22 ~ ArTéMiS 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. MIETTINEN O., MATTERN M. and ANDRE P.

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