|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| WR 93b , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST13:23:39 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2004MNRAS.351..206D | 37 | K | 14 | 19 | Discovery of a WO star in the Scutum-Crux arm of the inner Galaxy. | DREW J.E., BARLOW M.J., UNRUH Y.C., et al. | |||
| 2005MNRAS.363..857H | 25 | 11 | Five WC9 stars discovered in the AAO/UKST Hα survey. | HOPEWELL E.C., BARLOW M.J., DREW J.E., et al. | |||||
| 2006A&A...449..711C | 83 | 129 | Reduced Wolf-Rayet line luminosities at low metallicity. | CROWTHER P.A. and HADFIELD L.J. | |||||
|
2006A&A...458..453V |
15 | D | 1 | 126 | 78 | New Galactic Wolf-Rayet stars, and candidates. An annex to The VIIth Catalogue of Galactic Wolf-Rayet Stars. | VAN DER HUCHT K.A. | ||
| 2007ARA&A..45..177C | 5 | 51 | 776 | Physical properties of Wolf-Rayet stars. | CROWTHER P.A. | ||||
| 2009A&A...502..611G | 19 | D | 2 | 16 | 149 | The different progenitors of type Ib, IC SNe, and of GRB. | GEORGY C., MEYNET G., WALDER R., et al. | ||
|
2010ApJS..191..301A |
90 | D | C | 3 | 173 | 21 | The Spitzer atlas of stellar spectra (SASS). | ARDILA D.R., VAN DYK S.D., MAKOWIECKI W., et al. | |
|
2013A&A...558A.131G |
193 | X C | 4 | 60 | 160 | Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death. | GROH J.H., MEYNET G., GEORGY C., et al. | ||
| 2013A&A...559A..72T | 38 | X | 1 | 16 | 23 | On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613. | TRAMPER F., GRAEFENER G., HARTOOG O.E., et al. | ||
| 2015A&A...581A.110T | 875 | D | O X C | 22 | 18 | 56 | Massive stars on the verge of exploding: the properties of oxygen sequence Wolf-Rayet stars. | TRAMPER F., STRAAL S.M., SANYAL D., et al. | |
| 2016ApJ...833..133T | 16 | D | 1 | 24 | 8 | A new prescription for the mass-loss rates of WC and WO stars. | TRAMPER F., SANA H. and DE KOTER A. | ||
| 2018MNRAS.473..447L | 80 | X | 2 | 23 | 1 | Rontgen spheres around active stars. | LOCCI D., CECCHI-PESTELLINI C., MICELA G., et al. | ||
| 2018MNRAS.473.2853R | 16 | D | 1 | 302 | 7 | A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars. | ROSSLOWE C.K. and CROWTHER P.A. | ||
| 2018MNRAS.479.4535S | 2569 | A | D | S X C F | 62 | 11 | 5 | Probing the rotational velocity of Galactic WO stars with spectropolarimetry. | STEVANCE H.F., IGNACE R., CROWTHER P.A., et al. |
| 2019A&A...621A..92S | 284 | X C | 6 | 72 | 69 | The Galactic WC and WO stars. The impact of revised distances from Gaia DR2 and their role as massive black hole progenitors. | SANDER A.A.C., HAMANN W.-R., TODT H., et al. | ||
|
2020MNRAS.493.1512R |
16 | D | 1 | 393 | 47 | Unlocking Galactic Wolf-Rayet stars with Gaia DR2 - I. Distances and absolute magnitudes. | RATE G. and CROWTHER P.A. | ||
| 2022A&A...658A..46A | 783 | D | X C | 18 | 3 | ~ | Intrinsic polarization of Wolf-Rayet stars due to the rotational modulation of the stellar wind. | ABDELLAOUI S., KRTICKA J. and KURFURST P. | |
| 2023MNRAS.521..585C | 148 | D | X F | 3 | 274 | 1 | Line luminosities of Galactic and Magellanic Cloud Wolf-Rayet stars. | CROWTHER P.A., RATE G. and BESTENLEHNER J.M. | |
| 2023MNRAS.523.2530D | 44 | X | 1 | 19 | 6 | SN 2022ann: a Type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environment. | DAVIS K.W., TAGGART K., TINYANONT S., et al. | ||
|
2025A&A...695A.227M |
47 | X | 1 | 80 | ~ | Search for new Galactic Wolf-Rayet stars using Gaia DR3 I. Candidate selection and the follow-up of the bright sample. | MULATO L., MERC J., CHARBONNEL S., et al. | ||
| 2025A&A...698A.225A | 392 | D | X C | 8 | 4 | ~ | Polarization of light from fast-rotating Wolf-Rayet stars: Monte Carlo simulations compared to the analytical formula. | ABDELLAOUI S., KRTICKA J., KUBATOVA B., et al. |