|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| IRAS 18384-3310 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST21:49:11 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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 | ||
| 2008MNRAS.383..399L | 15 | D | 4 | 44 | 30 | Dust mass-loss rates from asymptotic giant branch stars in the Fornax and Sagittarius dwarf spheroidal galaxies. | LAGADEC E., ZIJLSTRA A.A., MATSUURA M., et al. | ||
| 2009MNRAS.396..598L | 727 | D | X C F | 18 | 24 | 20 | Metal-rich carbon stars in the Sagittarius dwarf spheroidal galaxy. | LAGADEC E., ZIJLSTRA A.A., SLOAN G.C., et al. | |
| 2012MNRAS.427.2588L | 244 | D | X | 7 | 20 | 5 | Dust and gas in carbon stars towards the Galactic halo. | LAGADEC E., SLOAN G.C., ZIJLSTRA A.A., et al. | |
|
2019A&A...626A..92G |
97 | D | X | 3 | 225 | ~ | 30-micron sources in galaxies with different metallicities. | GLADKOWSKI M., SZCZERBA R., SLOAN G.C., et al. | |
|
2022ApJS..260...46I |
17 | D | 1 | 65989 | 11 | The OGLE Collection of Variable Stars: Nearly 66,000 Mira Stars in the Milky Way. | IWANEK P., SOSZYNSKI I., KOZLOWSKI S., et al. | ||
|
2023ApJS..264...20I |
17 | D | 1 | 65989 | 1 | A Three-dimensional Map of the Milky Way Using 66,000 Mira Variable Stars. | IWANEK P., POLESKI R., KOZLOWSKI S., et al. | ||
|
2023A&A...674A..15L |
17 | D | 1 | 1720610 | 15 | Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. | LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al. | ||
|
2024ApJS..272...16S |
18 | D | 1 | 7259 | ~ | Infrared Properties of Carbon Stars in Our Galaxy. | SUH K.-W. |