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| IRAS 20180+3558 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST23:39:10 |
| 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...65..607O | 5415 | 387 | IRAS catalogues and atlases. Atlas of Low-Resolution Spectra. | OLNON F.M., RAIMOND E. (The IRAS Science Team) | |||||
| 1987ApJ...315..654V | 468 | 41 | On the contribution of interstellar extinction to the 10 micron dust feature in OH/IR stars. | VOLK K. and KWOK S. | |||||
|
1988IRASP.C......0J |
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...246..249P | 259 | 201 | Water masers associated with dense molecular clouds and ultracompact HII regions. | PALLA F., BRAND J., CESARONI R., et al. | |||||
|
1994ApJS...93..549L |
269 | 40 | Supplement to the Arecibo 1612 MHz survey of color-selected IRAS sources. | LEWIS B.M. | |||||
|
1996A&A...308..573M |
248 | 318 | A search for precursors of ultracompact HII regions in a sample of luminous IRAS sources. I. Association with ammonia cores. | MOLINARI S., BRAND J., CESARONI R., et al. | |||||
| 1997ApJS..111..387C | 39 | 84 | The high-resolution IRAS galaxy atlas. | CAO Y., TEREBEY S., PRINCE T.A., et al. | |||||
|
1997ApJS..112..557K |
11276 | 205 | Classification and identification of IRAS sources with low-resolution spectra. | KWOK S., VOLK K. and BIDELMAN W.P. | |||||
|
2000A&AS..143..269S |
1601 | 191 | A survey of the 6.7 GHz methanol maser emission from IRAS sources. I. Data. | SZYMCZAK M., HRYNEK G. and KUS A.J. | |||||
|
2007A&A...465..865E |
O | 230 | 33 | A survey of OH masers towards high mass protostellar objects. | EDRIS K.A., FULLER G.A. and COHEN R.J. | ||||
| 2010A&A...517A..56F | 15 | D | 1 | 307 | 67 | Class I and class II methanol masers in high-mass star-forming regions. | FONTANI F., CESARONI R. and FURUYA R.S. |