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| EM* MWC 685 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST18:56:30 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1935BSD...C01....0S | 13 | D | 1 | 1387 | ~ | Bergedorfer spektral-Durchmusterung der 115 Nordlichen Kapteynschen Eichfelder 1-19. | SCHWASSMANN A. and VAN RHIJN P.J. | ||
| 1949ApJ...110..387M | 445 | 193 | Second supplement to the Mount Wilson catalogue and bibliography of stars of classes B and A whose spectra have bright hydrogen lines. | MERRILL P.W. and BURWELL C.G. | |||||
| 1992A&AS...95..391M | 46 | 2 | New probable members of the young Orion stellar population. I. The obscured regions in Cassiopeia, Vela and Scorpius. | MARQUEZ-LIMON A., LOPEZ-MOLINA M.G. and CHAVARRIA-K C. | |||||
1997AAHam..11....1K 
|
4093 | ~ | Catalogue of stars in the Northern Milky Way having H-α in emission. | KOHOUTEK L. and WEHMEYER R. | |||||
|
1999A&AS..134..255K
|
4182 | 102 | Catalogue of H-alpha emission stars in the Northern Milky Way. | KOHOUTEK L. and WEHMEYER R. | |||||
|
2016MNRAS.463.1162C
|
16 | D | 1 | 1984 | 1 | A new approach to the infrared photometric study of Be stars. | CHEN P.S., LIU J.Y. and SHAN H.G. | ||
|
2017AJ....153..252L
|
16 | D | 1 | 588 | 56 | Photometric variability of the Be star population. | LABADIE-BARTZ J., PEPPER J., McSWAIN M.V., et al. | ||
|
2019MNRAS.490.3158C
|
17 | D | 1 | 465834 | 28 | A catalogue of stellar diameters and fluxes for mid-infrared interferometry. | CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al. | ||
|
2020A&A...641A..42B
|
17 | D | 1 | 510 | 42 | Investigating the lack of main-sequence companions to massive Be stars. | BODENSTEINER J., SHENAR T. and SANA H. | ||
|
2021A&A...645L...8X
|
17 | D | 1 | 9593 | 36 | Local spiral structure based on the Gaia EDR3 parallaxes. | XU Y., HOU L.G., BIAN S.B., et al. |
