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| [ABB2014] WISE G354.175-00.062 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST03:58:07 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2007ApJ...670..428C 
|
15 | D | 1 | 272 | 181 | The bubbling galactic disk. II. The inner 20°. | CHURCHWELL E., WATSON D.F., POVICH M.S., et al. | ||
|
2012MNRAS.424.2442S
|
15 | D | 1 | 5154 | 176 | The Milky Way Project First Data Release: a bubblier Galactic disc. | SIMPSON R.J., POVICH M.S., KENDREW S., et al. | ||
|
2014MNRAS.438..426H
|
15 | D | 1 | 834 | 10 | A statistical study of gaseous environment of Spitzer interstellar bubbles. | HOU L.G. and GAO X.Y. | ||
| 2014ApJS..214....3B | 15 | 10 | The Milky Way Project: leveraging citizen science and machine learning to detect interstellar bubbles. | BEAUMONT C.N., GOODMAN A.A., KENDREW S., et al. | |||||
| 2016PASJ...68...37H | 16 | D | 3 | 207 | 11 | Mid- and far-infrared properties of Spitzer Galactic bubbles revealed by the AKARI all-sky surveys. | HATTORI Y., KANEDA H., ISHIHARA D., et al. | ||
| 2017MNRAS.472.4750D | 2383 | T K A | D | S X C | 58 | 16 | 6 |
Infrared dust bubble CS51 and its interaction with the surrounding interstellar medium. |
DAS S.R., TEJ A., VIG S., et al. |
|
2019MNRAS.488.1141J
|
16 | D | 1 | 2612 | 20 | The Milky Way Project second data release: bubbles and bow shocks. | JAYASINGHE T., DIXON D., POVICH M.S., et al. | ||
|
2019PASJ...71....6H
|
97 | D | F | 6 | 321 | 9 | A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel. | HANAOKA M., KANEDA H., SUZUKI T., et al. | |
| 2022MNRAS.510..658P | 43 | X | 1 | 15 | 2 | Galactic H II region IRAS 17149 - 3916 - a multiwavelength study. | POTDAR A., DAS S.R., ISSAC N., et al. | ||
| 2024ApJ...974...10O | 18 | D | 1 | 173 | ~ | Implications for Galactic Electron Density Structure from Pulsar Sightlines Intersecting H II Regions. | OCKER S.K., ANDERSON L.D., LAZIO T.J.W., et al. |
