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相关论文: The Fossil Starburst in M82

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Using new HST imaging, we identify a large, evolved system of super star clusters in a disk region just outside the starburst core in the prototypical starburst galaxy M82, ``M82 B.'' This region has been suspected to be a fossil starburst…

天体物理学 · 物理学 2007-05-23 R. de Grijs , R. W. O'Connell , J. S. Gallagher

We present observations obtained with the Advanced Camera for Surveys on board the Hubble Space Telescope of the "fossil" starburst region B in the nearby starburst galaxy M82. By comparing UBVI photometry with models, we derive ages and…

We present a photometric study of star clusters in the nearby starburst galaxy M82 based on the UBVI, YJ and H band Hubble Space Telescope images. We find 1105 star clusters with V<23 mag. 1070 of them are located in the disk region, while…

宇宙学与河外天体物理 · 物理学 2015-06-12 Sungsoon Lim , Narae Hwang , Myung Gyoon Lee

We present high-resolution optical and near-infrared HST observations of two adjacent regions in the fossil starburst region in M82, B1 and B2. Age estimates date the cluster population in the fossil starburst between ~2 x 10^8 and ~10 x…

天体物理学 · 物理学 2007-05-23 R. de Grijs , R. W. O'Connell , J. S. Gallagher

We present optical spectroscopy obtained with the Space Telescope Imaging Spectrograph (STIS) of five young massive star clusters in the starburst galaxy M82. A detailed analysis is performed for one cluster `M82-A1' and its immediate…

天体物理学 · 物理学 2009-11-11 L. J. Smith , M. S. Westmoquette , J. S. Gallagher , R. W. O'Connell , D. J. Rosario , R. de Grijs

We present high-resolution optical and near-infrared HST observations of two adjacent regions in the fossil starburst region in M82, M82 B1 and B2. The presence of both the active and the fossil starburst in M82 provides a unique physical…

天体物理学 · 物理学 2009-10-31 Richard de Grijs , Robert W. O'Connell , John S. Gallagher

We present a spectroscopic study of the stellar cluster population of M82, the archetype starburst galaxy, based primarily on new Gemini-North multi-object spectroscopy of 49 star clusters. These observations constitute the largest to date…

星系天体物理 · 物理学 2009-08-05 I. S. Konstantopoulos , N. Bastian , L. J. Smith , M. S. Westmoquette , G. Trancho , J. S. Gallagher

The post-starburst region B in M82 and its massive star cluster component have been the focus of multiple studies, with reports that there is a large population of coeval clusters of age ~1 Gyr, which were created with a Gaussian initial…

天体物理学 · 物理学 2009-12-04 I. S. Konstantopoulos , N. Bastian , L. J. Smith , G. Trancho , M. S. Westmoquette , J. S. Gallagher

We present high signal-to-noise optical spectra of two luminous super star clusters in the starburst galaxy M82. The data for cluster F and the nearby, highly reddened cluster L were obtained with the William Herschel Telescope (WHT) at a…

天体物理学 · 物理学 2012-08-27 John S. Gallagher , III , Linda J. Smith

We analyse high-resolution Hubble Space Telescope/Advanced Camera for Surveys imaging of the nuclear starburst region of M82, obtained as part of the Hubble Heritage mosaic made of this galaxy, in four filters (Johnson-Cousins equivalent B,…

天体物理学 · 物理学 2009-11-13 S. Barker , R. de Grijs , M. Cervino

Recent HST/ACS images of M82 covering the entire galaxy have been used to detect star clusters. The galaxy is known to contain a young population (age < 10 Myr) in its starburst nucleus, surrounded by a post-starburst disk of age < 1 Gyr.…

天体物理学 · 物理学 2007-10-12 Y. D. Mayya , D. Rosa-Gonzalez , L. Rodriguez , L. Carrasco , R. Romano , A. Luna

Using high-resolution, multiple-passband Hubble Space Telescope images spanning the entire optical/near-infrared wavelength range, we obtained a statistically complete sample, $U$-band selected sample of 846 extended star clusters across…

星系天体物理 · 物理学 2015-06-23 Shuo Li , Richard de Grijs , Peter Anders , Chengyuan Li

We present new spectroscopic observations of the stellar cluster population of region B in the prototype starburst galaxy M82 obtained with the Gillett Gemini-North 8.1-metre telescope. By coupling the spectroscopy with UBVI photometry…

天体物理学 · 物理学 2011-10-05 I. S. Konstantopoulos , N. Bastian , L. J. Smith , G. Trancho , M. S. Westmoquette , J. S. Gallagher

We report the discovery of ten compact H-alpha-bright sources in the post-starburst region northeast of the center of M82, ``M82 B.'' These objects have H alpha luminosities and sizes consistent with Type II supernova remnants (SNRs). They…

M82 B is an old starburst site located in the eastern part of the M82 disc. We derive the distributions of age and metallicity of the star clusters located in this region of M82 by using theoretical evolutionary population synthesis models.…

天体物理学 · 物理学 2009-11-07 G. Parmentier , R. de Grijs , G. Gilmore

Recent results from Hubble Space Telescope (HST) have resolved starbursts as collections of compact young stellar clusters. Here we present a photometric catalogue of the young stellar clusters in the nuclear starburst of M82, observed with…

天体物理学 · 物理学 2016-08-16 V. P. Melo , C. Muñoz-Tuñón , J. Maíz-Apellániz , G. Tenorio-Tagle

We present the results obtained from an objective search for stellar clusters, both in the currently active nuclear starburst region, and in the post-starburst disk of M82. Images obtained with the HST/ACS in F435W(B), F555W(V), and…

天体物理学 · 物理学 2009-11-13 Y. D. Mayya , R. Romano , L. H. Rodriguez-Merino , A. Luna , L. Carrasco , D. Rosa-Gonzalez

We present HST/STIS optical and Gemini/NIFS near-IR IFU spectroscopy, and archival HST imaging of the triplet of super star clusters (A1, A2 and A3) in the core of the M82 starburst. Using model fits to the STIS spectra, and the weakness of…

We present a near infrared (NIR) candidate star cluster catalog for the central kiloparsec of M82 based on new JWST NIRCam images. We identify star cluster candidates using the F250M filter, finding 1357 star cluster candidates with stellar…

M82 is the nearest starburst galaxy. It contains two large systems of super star clusters, one being spawned today in the active starforming core, and one produced by an earlier starburst event which coincided with the last orbital passage…

天体物理学 · 物理学 2007-05-23 Robert W. O'Connell
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