|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| DCld 301.6-07.8 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:32:23 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1986A&AS...63...27H |
1095 | 135 | A catalogue of southern dark clouds. | HARTLEY M., MANCHESTER R.N., SMITH R.M., et al. | |||||
| 1988A&AS...76..347G | 94 | 58 | Star counts and IRAS sources in the southern dark clouds. | GREGORIO-HETEM J.C., SANZOVO G.C. and LEPINE J.R.D. | |||||
|
2000MNRAS.317...55S |
14 | D | 1 | 16424 | 457 | The PSCz catalogue. | SAUNDERS W., SUTHERLAND W.J., MADDOX S.J., et al. | ||
|
2000PASA...17...92O |
1093 | 19 | Catalogue of J = 1-0 CO emission towards southern dark clouds. | OTRUPCEK R.E., HARTLEY M. and WANG J.-S. | |||||
| 2001PASJ...53.1071M | 28 | 43 | A large scale ^12CO (J = 1–0) survey toward the Chamaeleon region with NANTEN. | MIZUNO A., YAMAGUCHI R., TACHIHARA K., et al. | |||||
|
2002A&A...383..631D |
14 | D | 3330 | 41 | A catalogue of dust clouds in the Galaxy. | DUTRA C.M. and BICA E. | |||
|
2004ApJ...603..584P |
26 | 48 | Polarimetry toward the Musca dark cloud. I. The catalog. | PEREYRA A. and MAGALHAES A.M. | |||||
|
2011PASJ...63S...1D |
15 | D | 1 | 7614 | 100 | Atlas and Catalog of Dark Clouds Based on the 2 Micron All Sky Survey. | DOBASHI K. | ||
| 2016A&A...587A..97H | 239 | O X C | 5 | 12 | 79 | The Musca cloud: A 6 pc-long velocity-coherent, sonic filament. | HACAR A., KAINULAINEN J., TAFALLA M., et al. | ||
| 2016A&A...590A.110C | 43 | X | 1 | 11 | 100 | Filamentary structure and magnetic field orientation in Musca. | COX N.L.J., ARZOUMANIAN D., ANDRE P., et al. | ||
| 2017ApJ...836...19M | 302 | A | X C | 7 | 13 | 1 | Properties of dense cores embedded in Musca derived from extinction maps and 13CO, C18O, and NH3 emission lines. | MACHAIEIE D.A., VILAS-BOAS J.W., WUENSCHE C.A., et al. |