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相关论文: The NGC 7742 star cluster luminosity function: A p…

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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 young populous cluster NGC 1866 in the Large Magellanic Cloud LMC), which is probably one of the most massive object formed in the LMC during the last ~ 3 Gyr, appears to have an unexpectedly high mass-to-light ratio. From its velocity…

天体物理学 · 物理学 2009-10-31 Sidney van den Bergh

We present UBVRI photometry of the open cluster NGC 2422 (age $\sim 10^8$ yr) down to a limiting magnitude $V\simeq19$. These data are used to derive the Luminosity and Mass Functions and to study the cluster spatial distribution. By…

天体物理学 · 物理学 2008-11-26 L. Prisinzano , G. Micela , S. Sciortino , F. Favata

The supermassive black hole at the center of the Milky Way plays host to a massive, young cluster that may have formed in one of the most inhospitable environments in the Galaxy. We present new measurements of the global properties of this…

太阳与恒星天体物理 · 物理学 2015-06-12 Jessica R. Lu , Tuan Do , Andrea M. Ghez , Mark R. Morris , Sylvana Yelda , Keith Matthews

We use the Advanced Camera for Surveys on the Hubble Space Telescope to study the rich population of young massive star clusters in the main body of NGC 3256, a merging pair of galaxies with a high star formation rate (SFR) and SFR per unit…

星系天体物理 · 物理学 2016-07-27 Alexander J. Mulia , Rupali Chandar , Bradley C. Whitmore

We performed a HST/WFC3-IR imaging survey of the young stellar cluster NGC 2024 in three filters probing the 1.4~$\mu$m H$_2$O absorption feature, characteristic of the population of low mass and sub-stellar mass objects down to a few…

We examine star clusters in the irregular, starburst galaxy NGC 1569 from HST images. In addition to the two known super star clusters, we identify 45 other clusters that are compact but resolved. Integrated UVI colors of the clusters span…

天体物理学 · 物理学 2009-10-31 D. A. Hunter , R. W. O'Connell , J. S. Gallagher , T. A. Smecker-Hane

We have used previously published observations of the CO emission from the Antennae (NGC 4038/39) to study the detailed properties of the super giant molecular complexes with the goal of understanding the formation of young massive star…

天体物理学 · 物理学 2009-11-10 C. D. Wilson , N. Z. Scoville , S. C. Madden , V. Charmandaris

Deep HST-WFPC2 observations of the stellar population in the globular cluster Omega Cen (NGC 5139) have been used to measure the luminosity function of main sequence stars at the low-mass end. Two fields have been investigated, located…

天体物理学 · 物理学 2009-10-31 Guido De Marchi

Based on deep VLT/ISAAC JHK photometry, we have derived the present-day mass function of the central starburst cluster NGC 3603 YC (Young Cluster) in the giant HII region NGC 3603. The effects of field contamination, individual reddening,…

天体物理学 · 物理学 2008-11-26 Andrea Stolte , Wolfgang Brandner , Bernhard Brandl , Hans Zinnecker

We present {\it Hubble Space Telescope} {\it V,I} photometry of the central region of the LMC cluster NGC 1866, reaching magnitudes as faint as V=27 mag. We find evidence that the cluster luminosity function shows a strong dependence on the…

天体物理学 · 物理学 2009-11-07 E. Brocato , V. Castellani , E. Di Carlo , G. Raimondo , A. R. Walker

We test claims that the power-law mass functions of young star clusters (ages $\lesssim\mbox{few}\times10^8$~yr) have physical upper cutoffs at $M_*\sim10^5~M_{\odot}$. Specifically, we perform maximum-likelihood fits of the Schechter…

星系天体物理 · 物理学 2019-02-20 Angus Mok , Rupali Chandar , S. Michael Fall

We present a principal component analysis of galaxy spectra from the CNOC sample of rich X-ray luminous clusters at 0.18 < z < 0.55. Composite radial distributions of different stellar populations show strong gradients as a function of…

天体物理学 · 物理学 2007-05-23 E. Ellingson , H. Lin , H. K. C. Yee , R. G. Carlberg

We present the luminosity function (LF) of star clusters in M51 based on HST/ACS observations taken as part of the Hubble Heritage project. The clusters are selected based on their size and with the resulting 5990 clusters we present one of…

天体物理学 · 物理学 2009-11-11 Mark Gieles , Soeren Larsen , Remco Scheepmaker , Nate Bastian , Marcel Haas , Henny Lamers

In this paper we derive ages and masses for 276 clusters in the merger galaxy NGC 3256. This was achieved by taking accurate photometry in four wavebands from archival HST images. Photometric measurements are compared to synthetic stellar…

宇宙学与河外天体物理 · 物理学 2015-05-18 Q. E. Goddard , N. Bastian , R. C. Kennicutt

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

The spatial morphology and dynamical status of a young, still-forming stellar cluster provide valuable clues on the conditions during the star formation event and the processes that regulated it. We analyze the Orion Nebula Cluster (ONC),…

星系天体物理 · 物理学 2015-06-22 Nicola Da Rio , Jonathan C. Tan , Karl Jaehnig

We explore the near-infrared properties of galaxies within 27 galaxy clusters using data from the Two Micron All Sky Survey (2MASS). For a subsample of 13 clusters with available X-ray imaging data, we examine both the properties of the…

天体物理学 · 物理学 2009-11-07 Yen-Ting Lin , Joseph J. Mohr , S. A. Stanford

We present the I-band luminosity function of the differentially reddened globular cluster M10. We combine photometric analysis derived from wide-field (23' x 23') images that include the outer regions of the cluster and high-resolution…

天体物理学 · 物理学 2016-08-30 Denise L. Pollard , Eric L. Sandquist , Jonathan R. Hargis , Michael Bolte

We have used the NASA Infra-Red Telescope Facility (IRTF) to observe the nuclear stellar cluster in the nearby, face-on, giant Scd spiral IC 342. From high resolution (R = 21500) spectra at the 12CO (2-0) bandhead at 2.3 micron we derive a…

天体物理学 · 物理学 2009-10-31 T. Boeker , R. P. van der Marel , W. D. Vacca