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相关论文: The Young Cluster Population of M82 Region B

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(Abridged) We present high-resolution HST imaging in the optical (WFPC2) and near-infrared (NICMOS) of a disk region 1 kpc NE of the starburst core in the nearby galaxy M82. This region, M82 ``B,'' has been suspected to be a fossil…

天体物理学 · 物理学 2019-08-17 Richard de Grijs , Robert W. O'Connell , John S. Gallagher , III

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 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 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 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

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

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 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

ABRIDGED: We obtain new age and mass estimates for the star clusters in M82's fossil starburst region B, based on improved fitting methods. Our new age estimates confirm the peak in the age histogram attributed to the last tidal encounter…

天体物理学 · 物理学 2009-11-07 Richard de Grijs , Nate Bastian , Henny J. G. L. M. Lamers

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

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

The M82 galaxy has been the subject of several studies basically because it is relatively close to to the Milky Way and it displays a strong star formation activity. Using multi-band images of M82 we have determined the age and extinction…

宇宙学与河外天体物理 · 物理学 2009-06-04 L. H. Rodriguez-Merino , D. Rosa-Gonzalez , Y. D. Mayya , L. Carrasco , A. Luna , R. Romano

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

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 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 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 large majority of extragalactic star cluster studies done to date have essentially used two or three-passband aperture photometry, combined with theoretical stellar population synthesis models, to obtain age estimates. The accuracy to…

天体物理学 · 物理学 2009-11-07 Richard de Grijs

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 use archival {\it Hubble Space Telescope} observations of broad-band images from the ultraviolet (F255W-filter) through the near infrared (NICMOS F160W-filter) to study the star cluster population of the interacting spiral galaxy M51. We…

天体物理学 · 物理学 2009-11-10 N. Bastian , M. Gieles , H. J. G. L. M. Lamers , R. de Grijs , R. A. Scheepmaker

We present a HST multiband analysis of the large population of star clusters in the blue compact galaxy (BCG) Mrk 930. We have reconstructed the spectral energy distributions of the star clusters and estimated age, mass, and extinction for…

宇宙学与河外天体物理 · 物理学 2015-05-27 A. Adamo , G. Ostlin , E. Zackrisson , P. Papaderos , N. Bergvall , R. M. Rich , G. Micheva
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