CXOU J140429.1+542353 , the SIMBAD biblio

CXOU J140429.1+542353 , the SIMBAD biblio (37 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:59:18


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Title First 3 Authors
1985ApJ...290..449S 2 7 101 Spatial variations in the physical conditions in the giant extragalactic HII region NGC 5471. SKILLMAN E.D.
1986ApJ...311...85C 8 39 Kinematic detection of supernova remnants in giant HII regions. CHU Y.-H. and KENNICUTT R.C.Jr
1988IAUCo.101..201C 12 ~ Supernova remnants in giant HII regions. CHU Y.H. and KENNICUTT R.C.
1990RMxAA..21..223D 8 8 Abundance analysis of giant HII regions in nearby spirals. DIAZ A.I., TERLEVICH E., PAGEL B.E.J., et al.
1991MNRAS.249..722Y 1 14 62 A new study of N 66 in the Small Magellanic Cloud. YE T., TURTLE A.J. and KENNICUTT R.C.
1993ApJ...411..655S 6 11 294 Spatially resolved optical and near-infrared spectroscopy of I Zw 18. SKILLMAN E.D. and KENNICUTT R.C.
1994AJ....107..651Y 16 15 A kinematic search for supernova remnants in giant extragalactic H II regions. YANG H., SKILLMAN E.D. and SRAMEK R.A.
1996ApJ...456..504K 49 169 The composition gradient in M101 revisited. I. H II region spectra and excitation properties. KENNICUTT R.C.Jr and GARNETT D.R.
1999ApJ...517L..27W 2 7 54 Detection of x-ray-emitting hypernova remnants in M101. WANG Q.D.
1999ApJ...523..121W 83 40 An ultradeep high-resolution X-ray image of M101: the X-ray source population in a late-type spiral. WANG Q.D., IMMLER S.A. and PIETSCH W.
2000MNRAS.312..130D 141 87 An empirical calibration of nebular abundances based on the sulphur emission lines. DIAZ A.I. and PEREZ-MONTERO E.
2001AJ....121.3001S 9 15 Reconsidering the identification of M101 hypernova remnant candidates. SNOWDEN S.L., MUKAI K., PENCE W., et al.
2001ApJ...547..754L 29 14 A critical examination of hypernova remnant candidates in M101. I. MF 83. LAI S.-P., CHU Y.-H., CHEN C.-H.R., et al.
2002AJ....123.2462C 72 T                   46 20 A critical examination of hypernova remnant candidates in M101. II.
NGC 5471B.
CHEN C.-H.R., CHU Y.-H., GRUENDL R., et al.
2002MNRAS.329..481B 40 26 Narrow-band CCD photometry of giant H II regions. BOSCH G., TERLEVICH E. and TERLEVICH R.
2002MNRAS.330...69D 1 95 394 New light on the search for low-metallicity galaxies - I. The N2 calibrator. DENICOLO G., TERLEVICH R. and TERLEVICH E.
2003ApJ...591..801K 3 38 380 The composition gradient in M101 revisited. II. Electron temperatures and implications for the nebular abundance scale. KENNICUTT R.C.Jr, BRESOLIN F. and GARNETT D.R.
2004MNRAS.349..404J 52 24 An XMM-Newton view of M101 - I. The luminous X-ray source population. JENKINS L.P., ROBERTS T.P., WARWICK R.S., et al.
2005ApJ...619..779C 86 14 Clusters in the luminous giant H II regions in M 101. CHEN C.-H.R., CHU Y.-H. and JOHNSON K.E.
2005MNRAS.360..416L 93 23 Infrared mergers and infrared quasi-stellar objects with galactic winds - III. Mrk 231: an exploding young quasi-stellar object with composite outflow/broad absorption lines (and multiple expanding superbubbles). LIPARI S., TERLEVICH R., ZHENG W., et al.
2006A&A...449..193P 147 22 An empirical calibration of sulphur abundance in ionised gaseous nebulae. PEREZ-MONTERO E., DIAZ A.I., VILCHEZ J.M., et al.
2007AJ....133.1361P 59 21 A search for Chandra-detected X-ray counterparts to optically identified and candidate radio supernova remnants in five nearby face-on spiral galaxies. PANNUTI T.G., SCHLEGEL E.M. and LACEY C.K.
2007MNRAS.381L..26L 111           X         3 26 21 A synchrotron superbubble in the IC10 galaxy: a hypernova remnant? LOZINSKAYA T.A. and MOISEEV A.V.
2008AstL...34..217L 33 9 Synchrotron superbubble in the galaxy IC 10: The ionized gas structure, kinematics, and emission spectrum. LOZINSKAYA T.A., MOISEEV A.V., PODORVANYUK N.Y., et al.
2009ApJ...700..309B 76           X         2 76 224 Extragalactic chemical abundances: do H II regions and young stars tell the same story? the case of the spiral galaxy NGC 300. BRESOLIN F., GIEREN W., KUDRITZKI R.-P., et al.
2011AJ....141..126G viz 303           X C F     6 15 14 The 100 myr star formation history of NGC 5471 from cluster and resolved stellar photometry. GARCIA-BENITO R., PEREZ E., DIAZ A.I., et al.
2012AJ....143...85F 76           X         2 85 10 Physical structure and nature of supernova remnants in M101. FRANCHETTI N.A., GRUENDL R.A., CHU Y.-H., et al.
2012MNRAS.424.2316P viz 15       D               1 298 113 `Counterpart' method for abundance determinations in HII regions. PILYUGIN L.S., GREBEL E.K. and MATTSSON L.
2012ApJ...760...61S 969       D S   X C       24 29 2 Giant H II regions in M101. I. X-ray analysis of hot gas. SUN W., CHEN Y., FENG L., et al.
2015MNRAS.446..943V viz 39           X         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.
2016MNRAS.456.4407D viz 16       D               2 164 6 Sulphur abundance determinations in star-forming regions - I. Ionization correction factor. DORS O.L., PEREZ-MONTERO E., HAGELE G.F., et al.
2016PASJ...68S..18Y 39           X         1 14 ~ Iron emission line from the spiral galaxy M101. YAMAUCHI S.
2016MNRAS.460.1739V viz 16       D               1 615 58 BOND: Bayesian Oxygen and Nitrogen abundance Determinations in giant H II regions using strong and semistrong lines. VALE ASARI N., STASINSKA G., MORISSET C., et al.
2019ApJ...878...71L viz 41           X         1 165 5 Uncovering red and dusty ultraluminous X-ray sources with Spitzer. LAU R.M., HEIDA M., WALTON D.J., et al.
2020MNRAS.495.4347B 1095     A S   X C       25 23 ~ Internal kinematics of giant H II regions in M101 with the Keck Cosmic Web Imager. BRESOLIN F., RIZZI L., HO I.-T., et al.
2020MNRAS.497..672A viz 16       D               1 127 16 The Te[N II]-Te[O III] temperature relation in H II regions and the reliability of strong-line methods. ARELLANO-CORDOVA K.Z. and RODRIGUEZ M.
2024A&A...691A..70N 90           X         2 12 ~ Disruption of a massive molecular cloud by a supernova in the Galactic Centre Initial results from the ACES project. NONHEBEL M., BARNES A.T., IMMER K., et al.

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