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| [HJB85] Sgr A-H7 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:41:53 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1987ApJ...320..545Y | 1 | 33 | 195 | Structural details of the Sagittarius A complex: evidence for a large-scale poloidal magnetic field in the Galactic Center region. | YUSEF-ZADEH F. and MORRIS M. | ||||
| 1989ApJ...343..703M | 32 | 102 | The thermal, Arched filaments of the Radio Arc near the Galactic Center : magnetohydrodynamic-induced ionization ? | MORRIS M. and YUSEF-ZADEH F. | |||||
| 1993ApJ...418..235Z | 13 | 21 | VLA radio recombination line observations of ionized gas in the - 30 kilometers per second molecular cloud (G 0.04+0.03) near the Galactic Center. I. The discrete radio sources. | ZHAO J.-H., DESAI K., GOSS W.M., et al. | |||||
| 1999ApJ...510..747C | 39 | 53 | Isolated hot stars in the Galactic Center vicinity. | COTERA A.S., SIMPSON J.P., ERICKSON E.F., et al. | |||||
| 2000ApJS..129..123C | 24 | 27 | Interstellar extinction in the vicinity of the Galactic Center. | COTERA A.S., SIMPSON J.P., ERICKSON E.F., et al. | |||||
| 2001AJ....121.2681L | 17 | 39 | A VLA H92α recombination line study of the arched filament H II complex near the Galactic Center. | LANG C.C., GOSS W.M. and MORRIS M. | |||||
| 2003ApJ...598..325Y | 30 | 31 | The origin of the Galactic Center nonthermal radio filaments: young stellar clusters. | YUSEF-ZADEH F. | |||||
| 2007ApJ...662..574M | 35 | 24 | Discovery of hot supergiant stars near the Galactic Center. | MAUERHAN J.C., MUNO M.P. and MORRIS M. | |||||
| 2017MNRAS.470..561D | 199 | X F | 4 | 20 | 2 | IRTF/TEXES observations of the H II regions H1 and H2 in the Galactic Centre. | DONG H., LACY J.H., SCHODEL R., et al. | ||
| 2019ApJ...877...22H | 504 | D | X C | 12 | 58 | ~ | SOFIA/FORCAST observations of the Sgr A-H H II regions: using dust emission to elucidate the heating sources. | HANKINS M.J., LAU R.M., MILLS E.A.C., et al. |