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BA 1-416 , the SIMBAD biblio (26 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST23:31:09 |
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 |
---|---|---|---|---|---|---|---|---|---|
1964ApJ...139.1027B | 822 | 178 | Positions of emission nebulae in M 31. | BAADE W. and ARP H.C. | |||||
1978A&AS...31..439P | 14 | D | 1 | 984 | 140 | A survey of HII regions in M 31. | PELLET A., ASTIER N., VIALE A., et al. | ||
1980A&AS...40...67D | 66 | 142 | A catalogue of supernova remnant candidates in nearby galaxies. | D'ODORICO S., DOPITA M.A. and BENVENUTI P. | |||||
1980ApJ...236..628D | 19 | 77 | Optical emission from shocks. VI. Abundance gradient in M 33 from supernova remnants. | DOPITA M.A., D'ODORICO S. and BENVENUTI P. | |||||
1981ApJ...247..879B | 1 | 21 | 142 | Supernova remants in M 31. | BLAIR W.P., KIRSHNER R.P. and CHEVALIER R.A. | ||||
1982ApJ...254...50B | 1 | 36 | 195 | Abundance gradients in M 31: comparison of results from supernova remnants and HII regions. | BLAIR W.P., KIRSHNER R.P. and CHEVALIER R.A. | ||||
1984MNRAS.206..351D | 20 | 33 | Radio emission from supernova remnants in M 31 at a wavelength of 6 cm. | DICKEL J.R. and D'ODORICO S. | |||||
1990ApJS...72..761B | 540 | 33 | The interstellar medium of M 31. II. A survey of 20 centimeter continuum emission. | BRAUN R. | |||||
1997A&A...317..328S | 399 | 119 | ROSAT PSPC survey of M 31. | SUPPER R., HASINGER G., PIETSCH W., et al. | |||||
2001A&A...373...63S | 574 | 96 | The second ROSAT PSPC survey of M 31 and the complete ROSAT PSPC source list. | SUPPER R., HASINGER G., LEWIN W.H.G., et al. | |||||
2004ApJ...610..247D | 54 | 61 | Supersoft X-ray sources in M31. I. A Chandra survey and an extension to quasi-soft sources. | DI STEFANO R., KONG A.K.H., GREINER J., et al. | |||||
2005A&A...434..483P | 915 | 86 | An XMM-Newton survey of M 31. | PIETSCH W., FREYBERG M. and HABERL F. | |||||
2005A&A...435..437U | 162 | 26 | The Σ-D relation for supernova remnants in nearby galaxies. | UROSEVIC D., PANNUTI T.G., DURIC N., et al. | |||||
2006ApJ...643..844O | 56 | 29 | A close look at the population of supersoft and quasi-soft X-ray sources observed in M31 with XMM-Newton. | ORIO M. | |||||
2008A&A...480..599S | 15 | D | 317 | 21 | Time variability of X-ray sources in the M 31 centre field. | STIELE H., PIETSCH W., HABERL F., et al. | |||
2009A&A...495..733S | 15 | D | 1 | 339 | 8 | An X-ray spectral survey of the disc of M31 with XMM-Newton. | SHAW GREENING L., BARNARD R., KOLB U., et al. | ||
2010ApJ...717..739O | 123 | 25 | A census of the supersoft X-ray sources in M31. | ORIO M., NELSON T., BIANCHINI A., et al. | |||||
2011AJ....142..139A | 15 | D | 1 | 4380 | 79 | A new catalog of H II regions in M31. | AZIMLU M., MARCINIAK R. and BARMBY P. | ||
2011A&A...534A..55S | 15 | D | 1 | 2367 | 70 | The deep XMM-Newton survey of M 31. | STIELE H., PIETSCH W., HABERL F., et al. | ||
2012A&A...544A.144S | 39 | X | 1 | 47 | 15 | Supernova remnants and candidates detected in the XMM-Newton M31 large survey. | SASAKI M., PIETSCH W., HABERL F., et al. | ||
2012ApJ...761...26J | 15 | D | 1 | 67 | 30 | Supernova remnant progenitor masses in M31. | JENNINGS Z.G., WILLIAMS B.F., MURPHY J.W., et al. | ||
2012MNRAS.427.1463Z | 674 | D | X C | 17 | 49 | 110 | The chemical abundance in M31 from HII regions. | ZURITA A. and BRESOLIN F. | |
2014ApJ...786..130L | 16 | D | 1 | 208 | 28 | A new optical survey of supernova remnant candidates in M31. | LEE J.H. and LEE M.G. | ||
2015MNRAS.446..943V | 16 | D | 1 | 1179 | 6 | Optical supernova remnants in nearby galaxies and their influence on star formation rates derived from Hα emission. | VUCETIC M.M., ARBUTINA B. and UROSEVIC D. | ||
2018ApJ...861...92D | 16 | D | 1 | 65 | 11 | Progenitor mass distribution for core-collapse supernova remnants in M31 and M33. | DIAZ-RODRIGUEZ M., MURPHY J.W., RUBIN D.A., et al. | ||
2023ApJ...954..107C | 19 | D | 1 | 18 | ~ | A Nitrogen-rich Supernova Remnant in M31: Interaction with the Circumstellar Medium at Late Times. | CALDWELL N. and RAYMOND J.C. |