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| LGGS J013413.98+302759.0 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST01:32:34 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1982ApJS...49..405C | 266 | 84 | The cluster system of M 33. | CHRISTIAN C.A. and SCHOMMER R.A. | |||||
|
2007AJ....134..447S |
15 | D | 454 | 33 | A catalog of star cluster candidates in M 33. | SARAJEDINI A. and MANCONE C.L. | |||
|
2009ApJ...699..839S |
15 | D | 1 | 164 | 20 | Newly identified star clusters in M33. II. Radial Hubble space Telescope/Advanced camera for surveys fields. | SAN ROMAN I., SARAJEDINI A., GARNETT D.R., et al. | ||
|
2010ApJ...720.1674S |
15 | D | 2 | 2988 | 24 | Photometric properties of the M33 star cluster system. | SAN ROMAN I., SARAJEDINI A. and APARICIO A. | ||
|
2012ApJ...750...97D |
15 | D | 1 | 1241 | 71 | The yellow and red supergiants of M33. | DROUT M.R., MASSEY P. and MEYNET G. | ||
|
2012AJ....144...41M |
15 | D | 1 | 394 | 11 | An updated catalog of M33 clusters and candidates: UBVRI photometry and some statistical results. | MA J. | ||
|
2012MNRAS.426.2427S |
53 | D | X | 2 | 169 | 8 | Newly identified star clusters in M33 - III. Structural parameters. | SAN ROMAN I., SARAJEDINI A., HOLTZMAN J.A., et al. | |
|
2013AJ....145...88M |
15 | D | 1 | 460 | 6 | New UBVRI photometry of 234 M33 star clusters. | MA J. | ||
|
2014ApJS..211...22F |
15 | D | 1 | 716 | 14 | Star clusters in M33: updated UBVRI photometry, ages, metallicities, and masses. | FAN Z. and DE GRIJS R. | ||
|
2019ApJ...875..124N |
16 | D | 1 | 170 | 3 | Binary red supergiants. II. Discovering and characterizing B-type companions. | NEUGENT K.F., LEVESQUE E.M., MASSEY P., et al. | ||
|
2021ApJ...907...18R |
17 | D | 1 | 8559 | 15 | Red supergiants in M31 and M33. I. The complete sample. | REN Y., JIANG B., YANG M., et al. | ||
|
2021ApJ...912..112W |
17 | D | 1 | 3728 | 6 | Red supergiants in M31 and M33. II. The mass-loss rate. | WANG T., JIANG B., REN Y., et al. |