The M 4 Core Project with HST: I. Overview and first epoch
暂无分享,去创建一个
S. Ortolani | V. Nascimbeni | UCLA | STScI | G. Piotto | A. Bellini | D. C. Heggie | L. Malavolta | Harvard-Smithsonian CfA | Inc. | R. M. Rich | K. Brogaard | D. Heggie | Stsci | Ucla | R. Rich | G. Piotto | L. Malavolta | V. Nascimbeni | S. Ortolani | U. Victoria | Harvard-Smithsonian CfA | Iac | L. Úbeda | A. Milone | M. Giersz | U. Padova | U. Amsterdam | M. V. D. Berg | A. Bellini | K. Brogaard | A. Univ. | A. P. Milone | Univ. of Amsterdam | Eureka Scientific | M. Giersz | Eureka Scientific | IAC | U. L. Laguna | M. van den Berg | D. Pooley | L. Ubeda | L. R. Bedin J. Anderson | A. F. Marino . INAF-OAPD | Univ. of Edinburg | Univ. of Padova | Univ. of La Laguna | RSAA-ANU | N. Copernicus AC Warsaw | Sam Houston State Univ. | Aarhus Univ. | Univ. of Victoria | L. Anderson | D. Pooley | A. F. M. INAF-OAPD | N. Warsaw
[1] G. S. Burley,et al. THE CLUSTER AGES EXPERIMENT (CASE). V. ANALYSIS OF THREE ECLIPSING BINARIES IN THE GLOBULAR CLUSTER M4 , 2013, 1301.2946.
[2] David Charbonneau,et al. A Lack of Planets in 47 Tucanae from a Hubble Space Telescope Search , 2000 .
[3] Makino,et al. Astrophysics on the GRAPE family of special-purpose computers , 1999, Science.
[4] T. Fukushige,et al. The time-scale of escape from star clusters , 1999, astro-ph/9910468.
[5] J. Anderson,et al. A DOUBLE MAIN SEQUENCE IN THE GLOBULAR CLUSTER NGC 6397 , 2011, 1110.1077.
[6] S. Couch,et al. IDENTIFICATION OF FAINT CHANDRA X-RAY SOURCES IN THE CORE-COLLAPSED GLOBULAR CLUSTER NGC 6397: EVIDENCE FOR A BIMODAL CATACLYSMIC VARIABLE POPULATION , 2010, 1106.1927.
[7] J. Anderson,et al. The ACS survey of Galactic globular clusters. XII. Photometric binaries along the main sequence , 2011, 1111.0552.
[8] Douglas C. Heggie. The gravitational million-body problem , 2001 .
[9] G. Wallerstein,et al. High-resolution CCD spectra of stars in globular clusters. VII : Abundances of 16 elements in 47 Tuc, M4, and M22 , 1992 .
[10] J. Anderson,et al. Absolute motions of globular clusters - II. HST astrometry and VLT radial velocities in NGC 6397 , 2006, astro-ph/0605119.
[11] M. R. Haas,et al. PLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM KEPLER , 2011, 1103.2541.
[12] A. Schwarzenberg-Czerny,et al. Optimum Period Search: Quantitative Analysis , 1999 .
[13] Jay Anderson,et al. An Improved Distortion Solution for the Hubble Space Telescope’s WFPC2 , 2002 .
[14] H. Richer,et al. A Young White Dwarf Companion to Pulsar B1620-26: Evidence for Early Planet Formation , 2003, Science.
[15] M. Zechmeister,et al. The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms , 2009, 0901.2573.
[16] D. Heggie,et al. Monte Carlo simulations of star clusters – V. The globular cluster M4 , 2008 .
[17] V. Smith,et al. Star-to-Star Abundance Variations among Bright Giants in the Mildly Metal-poor Globular Cluster M4 , 1999, astro-ph/9905370.
[18] J. Hills. The formation of binaries containing black holes by the exchange of companions and the X-ray sources in globular clusters. , 1976 .
[19] Amsterdam,et al. X-Ray Sources and Their Optical Counterparts in the Globular Cluster M4 , 2004, astro-ph/0402197.
[20] Jay Anderson,et al. Toward High‐Precision Astrometry with WFPC2. I. Deriving an Accurate Point‐Spread Function , 2000, astro-ph/0006325.
[21] S. McMillan,et al. Formation and dynamical evolution of multiple stellar generations in globular clusters , 2008, 0809.1438.
[22] William E. Harris,et al. A Catalog of Parameters for Globular Clusters in the Milky Way , 1996 .
[23] B. Gibson,et al. Searching for Variability in the Globular Cluster Messier 4 , 2003, astro-ph/0304470.
[24] F. Rasio,et al. Stellar collisions during binary–binary and binary–single star interactions , 2004, astro-ph/0401004.
[25] Giampaolo Piotto,et al. Ground-based CCD astrometry with wide field imagers - I. Observations just a few years apart allow decontamination of field objects from members in two globular clusters , 2006 .
[26] J. Linsky,et al. The ROSAT All-Sky Survey of Active Binary Coronae. III. Quiescent Coronal Properties for the BY Draconis-Type Binaries , 1997 .
[27] C. Felix,et al. The molecular basis of leukemia. , 2004, Hematology. American Society of Hematology. Education Program.
[28] Giampaolo Piotto,et al. THE ACS SURVEY OF GLOBULAR CLUSTERS. V. GENERATING A COMPREHENSIVE STAR CATALOG FOR EACH CLUSTER , 2008 .
[29] S. Lucatello,et al. X-SHOOTER OBSERVATIONS OF MAIN-SEQUENCE STARS IN THE GLOBULAR CLUSTER NGC 2808: FIRST CHEMICAL TAGGING OF A He-NORMAL AND A He-RICH DWARF , 2010, 1007.5299.
[30] G. Piotto,et al. SODIUM–OXYGEN ANTICORRELATION AMONG HORIZONTAL BRANCH STARS IN THE GLOBULAR CLUSTER M4 , 2010, 1012.4931.
[31] D. Heggie,et al. Monte Carlo simulations of star clusters – VII. The globular cluster 47 Tuc , 2010, 1008.3048.
[32] G. Tagliaferri,et al. A CHANDRA X-RAY STUDY OF THE INTERACTING BINARIES IN THE OLD OPEN CLUSTER NGC 6791 , 2013, 1301.2331.
[33] STScI,et al. Astrometry and Photometry with HST WFC3. II. Improved Geometric-Distortion Corrections for 10 Filters of the UVIS Channel , 2011, 1102.5218.
[34] John Kormendy,et al. Inward Bound—The Search for Supermassive Black Holes in Galactic Nuclei , 1995 .
[35] J. Norris,et al. CN variations among asymptotic giant branch and horizontal branch stars in the intermediate metallicity globular clusters M5, M4, and NGC 6752 , 1993 .
[36] S. Anderson,et al. Addendum: “X-Ray Sources and Their Optical Counterparts in the Globular Cluster M4” (ApJ, 609, 755 [2004]) , 2005 .
[37] Jarrod R. Hurley,et al. Multiple stellar-mass black holes in globular clusters: theoretical confirmation , 2012, 1211.6608.
[38] R. Rich,et al. Probing the Faintest Stars in a Globular Star Cluster , 2006, Science.
[39] J. Norris. The cyanogen distribution of M4 and the possible connection between horizontal branch morphology and chemical inhomogeneity , 1981 .
[40] G. Piotto,et al. Color-Magnitude Diagram and Luminosity Function of M4 near the Hydrogen-burning Limit , 2001, astro-ph/0109059.
[41] I. Ram'irez,et al. TOWARD PRECISE AGES FOR SINGLE STARS IN THE FIELD. GYROCHRONOLOGY CONSTRAINTS AT SEVERAL Gyr USING WIDE BINARIES. I. AGES FOR INITIAL SAMPLE , 2011, 1109.0013.
[42] D. Geisler,et al. Bimodality of light and s-elements in M4 (NGC 6121) , 2011, 1109.0973.
[43] R. Rich,et al. An HST search for planets in the lower main sequence of the globular cluster NGC 6397 , 2012, 1202.5112.
[44] D. Heggie,et al. 1 Gyr in the life of the globular cluster NGC 6397 , 2009, 0904.4852.
[45] G. Piotto,et al. THE END OF THE WHITE DWARF COOLING SEQUENCE IN M4: AN EFFICIENT APPROACH , 2009, 0903.2839.
[46] L. Bedin,et al. Astrometry and Photometry with HST WFC3. I. Geometric Distortion Corrections of F225W, F275W, F336W Bands of the UVIS Channel , 2009, 0910.3250.
[47] K. Belczynski,et al. Formation and evolution of compact binaries in globular clusters – II. Binaries with neutron stars , 2007, 0706.4096.
[48] J. Anderson,et al. MULTIPLE STELLAR POPULATIONS IN 47 Tucanae , 2011, 1109.0900.
[49] Heidelberg,et al. The Frequency of Large-Radius Hot and Very Hot Jupiters in ω Centauri , 2007, 0710.3461.
[50] Ata Sarajedini,et al. The ACS Survey of Galactic Globular Clusters. I. Overview and Clusters without Previous Hubble Space Telescope Photometry , 2006, astro-ph/0612598.
[51] F. Grundahl,et al. Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. I. Measurements, methods, and first results , 2010, 1009.5537.
[52] V. Smith,et al. Sodium, aluminum, and oxygen abundance variations in giants in the globular cluster M4 , 1992 .
[53] J. Anderson,et al. Luminosity and mass functions of the three main sequences of the globular cluster NGC 2808 , 2011, 1108.2391.
[54] E. Vesperini,et al. Formation of Multiple Populations in Globular Clusters: constraints on the dilution by pristine gas , 2011, 1103.4715.
[55] Jay Anderson,et al. An Empirical Pixel-Based Correction for Imperfect CTE. I. HST’s Advanced Camera for Surveys , 2010, 1007.3987.
[56] D. Heggie,et al. MOCCA code for star cluster simulations II: comparison with n-body simulations , 2011, 1112.6246.
[57] A. Marín-Franch,et al. The ACS survey of Galactic globular clusters , 2012 .
[58] M. Giersz,et al. mocca code for star cluster simulations – I. Blue stragglers, first results , 2012, 1207.6700.
[59] Ji-Wei Xie,et al. Forming different planetary systems , 2012, 1207.2002.
[60] M. Inoue,et al. MULTI-FREQUENCY POLARIMETRY TOWARD S5 0836+710: A POSSIBLE SPINE–SHEATH STRUCTURE FOR THE JET , 2010 .
[61] S. Bogdanov,et al. A Deep Chandra Survey of the Globular Cluster 47 Tucanae: Catalog of Point Sources , 2005, astro-ph/0503132.
[62] K. Cunha,et al. Fluorine Abundance Variations in Red Giants of the Globular Cluster M4 and Early-Cluster Chemical Pollution , 2005, astro-ph/0506763.
[63] F. Grundahl,et al. Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members , 2010, Astronomy & Astrophysics.
[64] Johannes Andersen,et al. Accurate masses and radii of normal stars , 1991 .
[65] Jay Anderson,et al. The Rotation of the Globular Cluster 47 Tucanae in the Plane of the Sky , 2003 .
[66] Tomasz Bulik,et al. A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties , 2001, astro-ph/0111452.
[67] G. Piotto,et al. Spectroscopic and photometric evidence of two stellar populations in the Galactic globular cluster NGC 6121 (M 4) , 2008, 0808.1414.
[68] Australia.,et al. Monte Carlo simulations of star clusters -IV. Calibration of the Monte Carlo code and comparison with observations for the open cluster M67 , 2008, 0801.3709.
[69] P. Hut,et al. SUBMITTED TO APJL Preprint typeset using LATEX style emulateapj v. 6/22/04 DYNAMICAL FORMATION OF CLOSE BINARIES IN GLOBULAR CLUSTERS II: CATACLYSMIC VARIABLES , 2006 .
[70] D. Heggie,et al. Monte Carlo simulations of star clusters -VI. The globular cluster NGC 6397 , 2009, 0901.1085.
[71] Giampaolo Piotto,et al. Metallicities on the Double Main Sequence of ω Centauri Imply Large Helium Enhancement , 2004, astro-ph/0412016.
[72] A. Dotter,et al. A DEEP, WIDE-FIELD, AND PANCHROMATIC VIEW OF 47 Tuc AND THE SMC WITH HST: OBSERVATIONS AND DATA ANALYSIS METHODS , 2011, 1112.1426.
[73] B. Gibson,et al. The Lower Main Sequence and Mass Function of the Globular Cluster Messier 4 , 2002, astro-ph/0205086.
[74] K. Cudworth,et al. Radial velocities of stars in the globular cluster M4 and the cluster distance , 1995 .
[75] A. Gimenez,et al. Accurate masses and radii of normal stars: modern results and applications , 2009, 0908.2624.
[76] G. Carraro,et al. The absolute motion of the peculiar cluster NGC 6791 , 2006 .
[77] Scott Trager,et al. Catalogue of Galactic globular-cluster surface-brightness profiles , 1995 .
[78] S. Udry,et al. The road to Earth twins – Karl Schwarzschild Award Lecture 2010 , 2011 .
[79] Massimo Dall'Ora,et al. A NEW REDDENING LAW FOR M4 , 2012, 1204.5719.
[80] Transforming observational data and theoretical isochrones into the ACS/WFC Vega-mag system , 2004, astro-ph/0412328.
[81] R. Davies,et al. Neutral Hydrogen in the Galactic Region—II LOCATION OF THE EMISSION FEATURES , 1976 .
[82] J. Clausen. Eclipsing binaries as precise standard candles , 2004 .
[83] G. Kov'acs,et al. A box-fitting algorithm in the search for periodic transits , 2002, astro-ph/0206099.
[84] D. Pooley,et al. Globular cluster x-ray sources , 2004, astro-ph/0404136.
[85] Roeland P. van der Marel,et al. NEW LIMITS ON AN INTERMEDIATE-MASS BLACK HOLE IN OMEGA CENTAURI. I. HUBBLE SPACE TELESCOPE PHOTOMETRY AND PROPER MOTIONS , 2009, 0905.0627.
[86] D. Heggie,et al. A search for spectroscopic binaries in the Galactic globular cluster M4 Based on 5973 individual spectra collected at VLT , 2008, 0810.1897.