hit counter code 87+ 2002 Mnras - Height Distribution Of Black Hole X Ray Binaries, One Day Averaged RXTE ASM Light Curve KS 1947 300 During 2000 The 2 10 KeV Car Corrected For Instrumental, Amplitude Variations In Y 1987 Cycle D 1 Frequency 1995 And 2002

2002 Mnras

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KIAA Cambridge Workshop The Formation Of Peculiar Stars Zhanwen Han

KIAA Cambridge Workshop The Formation Of Peculiar Stars Zhanwen Han

The Group Of Bootis Stars Dr Ernst Paunzen Institute For Astronomy

The Group Of Bootis Stars Dr Ernst Paunzen Institute For Astronomy

The Various Angular Power Spectra Discussed In Text For Our Flat CDM Model

The Various Angular Power Spectra Discussed In Text For Our Flat CDM Model

Height Distribution Of Black Hole X Ray Binaries

Height Distribution Of Black Hole X Ray Binaries

One Day Averaged RXTE ASM Light Curve Of KS 1947 300 During 2000

One Day Averaged RXTE ASM Light Curve Of KS 1947 300 During 2000

The 2 10 KeV X Ray Light Curve Of Car Corrected For Instrumental

The 2 10 KeV X Ray Light Curve Of Car Corrected For Instrumental

Amplitude Variations In Y Of The 1987 Cycle D 1 Frequency During 1995 And 2002

Amplitude Variations In Y Of The 1987 Cycle D 1 Frequency During 1995 And 2002

The Location Of Masers Listed In Table 4 Superimposed On A Contour Plot

The Location Of Masers Listed In Table 4 Superimposed On A Contour Plot

Theoretical Estimates Of Intrinsic Galaxy Alignment

Theoretical Estimates Of Intrinsic Galaxy Alignment

The Molecular Fraction Versus Total NH Compared To Measurements In Magellanic Clouds

The Molecular Fraction Versus Total NH Compared To Measurements In Magellanic Clouds

9 SEDs Of L1544 L1498 Ward Thompson Et Al 2002 MNRAS 329 257

9 SEDs Of L1544 L1498 Ward Thompson Et Al 2002 MNRAS 329 257

Variability In Quiescent Black Holes

Variability In Quiescent Black Holes

This Shows The Distribution Of Faint And Bright Galaxies In One Strips Magnitude

This Shows The Distribution Of Faint And Bright Galaxies In One Strips Magnitude

Hubble Diagram For Quasar Surveys Used In The Paper I Isaak Et Al 2002

Hubble Diagram For Quasar Surveys Used In The Paper I Isaak Et Al 2002

17 GHz Phase Referenced And Self Calibrated Image Of NGC 3079

17 GHz Phase Referenced And Self Calibrated Image Of NGC 3079

Naturally Weighted Contour Map Of V404 Cyg As Observed By Westerbork At 49 GHz On 2002

Naturally Weighted Contour Map Of V404 Cyg As Observed By Westerbork At 49 GHz On 2002

The Region Around 4971 444 Showing OH Absorption From VLA 2002 Observation

The Region Around 4971 444 Showing OH Absorption From VLA 2002 Observation

Positions Of The 198 ERGs In CDFS Sample RDA03 Within Borders

Positions Of The 198 ERGs In CDFS Sample RDA03 Within Borders

Lindblad Torque On A Q 5 X 10 6 Planet Embedded In An Adiabatic Disc

Lindblad Torque On A Q 5 X 10 6 Planet Embedded In An Adiabatic Disc

Cumulative Distribution Of X Ray Sources As A Function The Luminosity

Cumulative Distribution Of X Ray Sources As A Function The Luminosity

Accreting Black Holes Should Have Been Detected By This Survey Given The Assumption Of Persistence We Can See Immediately From Fig

Accreting Black Holes Should Have Been Detected By This Survey Given The Assumption Of Persistence We Can See Immediately From Fig

Cumulative Distribution Of Observed And Simulated X Ray Sources As A Function The

Cumulative Distribution Of Observed And Simulated X Ray Sources As A Function The

The Observed Relation Between SFR Of A Galaxy And V Band Luminosity

The Observed Relation Between SFR Of A Galaxy And V Band Luminosity

Distribution Of The Minor To Major Axial Ratio A1 A3 In

Distribution Of The Minor To Major Axial Ratio A1 A3 In

White Dwarf Luminosity Functions Considering Different Evolutionary Stellar Models And Initial Final Mass Relationships

White Dwarf Luminosity Functions Considering Different Evolutionary Stellar Models And Initial Final Mass Relationships

Comparison Of The Rest Frame B Band LF Predicted By Our Simulation For Redshifts

Comparison Of The Rest Frame B Band LF Predicted By Our Simulation For Redshifts

The Light Curve Of SAX J18084 3658 During 2002 Outburst

The Light Curve Of SAX J18084 3658 During 2002 Outburst

23 GHz Phase Referenced And Self Calibrated Image Of NGC 3079

23 GHz Phase Referenced And Self Calibrated Image Of NGC 3079

The Differential V Band Luminosity Function Of Satellites Per Central Galaxy In Our Simulations

The Differential V Band Luminosity Function Of Satellites Per Central Galaxy In Our Simulations

Baryon Mass Profile According To Our Angular Momentum Prescription Solid Line Cf Equation

Baryon Mass Profile According To Our Angular Momentum Prescription Solid Line Cf Equation

The Positions Of Masers In Centre M82 Relation To H I

The Positions Of Masers In Centre M82 Relation To H I

Spectra Of Components A E F And B Measured In 2002 September

Spectra Of Components A E F And B Measured In 2002 September

The Radio Spectrum Of V404 Cyg As Measured By WSRT On 2001 December 28

The Radio Spectrum Of V404 Cyg As Measured By WSRT On 2001 December 28

PDF The Generation Of Dense Cores And Substructure Within Them By MHD Waves

PDF The Generation Of Dense Cores And Substructure Within Them By MHD Waves

M J Claussen NRAO H E Bond STScI K Healy And S

M J Claussen NRAO H E Bond STScI K Healy And S

Left Hand Graphs Sample Density Profiles Of B RGB And AGB Stars

Left Hand Graphs Sample Density Profiles Of B RGB And AGB Stars

Power Spectra And Fit Functions For 4U 1728 34 Top 0614

Power Spectra And Fit Functions For 4U 1728 34 Top 0614

A Comparison Between The Maser Velocities And Absorption Crosses Represent Measurements Of

A Comparison Between The Maser Velocities And Absorption Crosses Represent Measurements Of

The Location Of Main Line Masers In M82 With Other Features Shown For Comparison

The Location Of Main Line Masers In M82 With Other Features Shown For Comparison

Comparison Between IMFs For Several Young Clusters And Associations NGC 6611 This Work

Comparison Between IMFs For Several Young Clusters And Associations NGC 6611 This Work

Multiwavelength Light Curves For The Outburst Of Aql X 1 From 2002 March And

Multiwavelength Light Curves For The Outburst Of Aql X 1 From 2002 March And

Density Profiles For Model C 00025 Lines Are As In Fig

Density Profiles For Model C 00025 Lines Are As In Fig

Corrected Virial Mass Versus Stellar With A Variable Coefficient For Galaxies The Lower

Corrected Virial Mass Versus Stellar With A Variable Coefficient For Galaxies The Lower

The Observed Deprojected Spectrally Determined Temperature And Emission Measure Profiles For Abell 2199

The Observed Deprojected Spectrally Determined Temperature And Emission Measure Profiles For Abell 2199

Main Sequence Lifetime Versus Stellar Mass According To Different Authors Domnguez Et Al

Main Sequence Lifetime Versus Stellar Mass According To Different Authors Domnguez Et Al

CCDs For The Outbursts Of Aql X 1 From 2002 March Upper Left

CCDs For The Outbursts Of Aql X 1 From 2002 March Upper Left

Comparison Between The NIR Spectrum Of SN 2008ax Obtained On April 29 And Those

Comparison Between The NIR Spectrum Of SN 2008ax Obtained On April 29 And Those

Optical Apparent Magnitude SDSS I Band Versus Radio NVSS 1400 MHz

Optical Apparent Magnitude SDSS I Band Versus Radio NVSS 1400 MHz

The J 20 Mass Limit For Open Clusters From Dias Et Al 2002

The J 20 Mass Limit For Open Clusters From Dias Et Al 2002

The Best Fitting IMFs For ONC Muench Et Al 2002 Histogram

The Best Fitting IMFs For ONC Muench Et Al 2002 Histogram

Fig 1 Left Hubble Space Telescope Image Of The Gravitational Lensing System CLASS

Fig 1 Left Hubble Space Telescope Image Of The Gravitational Lensing System CLASS

Migration Time Scales For Different Sized Bodies In An Unperturbed Disc Ie No

Migration Time Scales For Different Sized Bodies In An Unperturbed Disc Ie No

Reproduction Of The X Ray Background Observations Are Highlighted By Shaded Areas And

Reproduction Of The X Ray Background Observations Are Highlighted By Shaded Areas And

IJHK Photometry For Our Compilation Of Pleiades BDs Excluding Those Objects Shown In Italics

IJHK Photometry For Our Compilation Of Pleiades BDs Excluding Those Objects Shown In Italics

John E Hibbard NRAO CV Interaction Driven Galaxy Evolution

John E Hibbard NRAO CV Interaction Driven Galaxy Evolution

2 Per Pixel Curves For Observed Data And Simulations Left Hand Side Fits

2 Per Pixel Curves For Observed Data And Simulations Left Hand Side Fits

The Cluster Velocity Dispersion As A Function Of Bolometric X Ray Luminosity

The Cluster Velocity Dispersion As A Function Of Bolometric X Ray Luminosity

Baryon Mass Profile According To Our Angular Momentum Prescription In Comparison With The Exponential Disc

Baryon Mass Profile According To Our Angular Momentum Prescription In Comparison With The Exponential Disc

Same As Fig 8 The Analytical Relation By Salpeter 1955 Solid Line

Same As Fig 8 The Analytical Relation By Salpeter 1955 Solid Line

The V Light Curve Of Z And During Its 2000 2002 Outburst Dots

The V Light Curve Of Z And During Its 2000 2002 Outburst Dots

True Colour Image From Our First Chandra ACIS S Observation 2002 December

True Colour Image From Our First Chandra ACIS S Observation 2002 December

Three Of The Central Masers In A Continuum Subtracted Single Channel From VLA 2002

Three Of The Central Masers In A Continuum Subtracted Single Channel From VLA 2002

Same As Fig 4 But Extending To Radio Frequencies And Showing Also Archival Data

Same As Fig 4 But Extending To Radio Frequencies And Showing Also Archival Data

The 850 M Number Counts N S As Determined From

The 850 M Number Counts N S As Determined From

Comparison Of The Predicted Galaxy Luminosity Functions Default Model With Hot Ram

Comparison Of The Predicted Galaxy Luminosity Functions Default Model With Hot Ram

Front X Ray Studies Of Galaxies And Galaxy Systems Jesper Rasmussen

Front X Ray Studies Of Galaxies And Galaxy Systems Jesper Rasmussen

The Observed G I Profiles Taken From SDSS Photometric Pipeline Stoughton Et Al

The Observed G I Profiles Taken From SDSS Photometric Pipeline Stoughton Et Al

Comparing LTIR Measured Using Three Different SED Models Chary Elbaz 2001 Dale

Comparing LTIR Measured Using Three Different SED Models Chary Elbaz 2001 Dale

Mass Distributions For White Dwarfs With Teff 12 000 K Considering Different Evolutionary Stellar Models

Mass Distributions For White Dwarfs With Teff 12 000 K Considering Different Evolutionary Stellar Models

The Data Used To Constrain Models Symbols Plus Errorbars And 68

The Data Used To Constrain Models Symbols Plus Errorbars And 68

The Luminosity Function Of Galaxies In Local Universe Upper Panel Compares Model

The Luminosity Function Of Galaxies In Local Universe Upper Panel Compares Model

Peak Flux Density Frequency And Time After Onset Of The Shock For Each

Peak Flux Density Frequency And Time After Onset Of The Shock For Each

The Physics Of Galaxy Formation Institute For Computational

The Physics Of Galaxy Formation Institute For Computational

K 12 Colour Versus M Giant Subtype Mass Loss Increases Towards Later

K 12 Colour Versus M Giant Subtype Mass Loss Increases Towards Later

The Visual Light Curve Of V838 Mon During First Three Months After Discovery Taken

The Visual Light Curve Of V838 Mon During First Three Months After Discovery Taken

7 XMM Newton Observations

7 XMM Newton Observations

Example Of A 2dF Spectrum With Poor Response At The Blue End In Top

Example Of A 2dF Spectrum With Poor Response At The Blue End In Top

CMD Used To Select The Boxes Size Of Was Determined By Requiring

CMD Used To Select The Boxes Size Of Was Determined By Requiring

A The Correlation Between Mass Accretion Rate And Stellar Previously Published Values

A The Correlation Between Mass Accretion Rate And Stellar Previously Published Values

The Raw White Light Curve For Reference And Target Star As Well

The Raw White Light Curve For Reference And Target Star As Well

The Location Of Main Line Masers Crosses Compared To SNRs From McDonald

The Location Of Main Line Masers Crosses Compared To SNRs From McDonald

Luminosity Temperature Relation The Line Is Best Fit For A Sample Of Optically

Luminosity Temperature Relation The Line Is Best Fit For A Sample Of Optically

The SFR As Estimated From Relation 8 In This Paper Blue Filled

The SFR As Estimated From Relation 8 In This Paper Blue Filled

6 FCvan Den Bosch 2002 MNRAS 332 456 Red Blue The Impact Of Cooling And Feed Back On Disc Galaxies

6 FCvan Den Bosch 2002 MNRAS 332 456 Red Blue The Impact Of Cooling And Feed Back On Disc Galaxies

Correlation Functions And Comparison With Other Work All For The Low Redshift Z

Correlation Functions And Comparison With Other Work All For The Low Redshift Z

Spectroscopic Evolution For A Representative Sample Of SNe Ibn The Spectra Are Reddening Corrected

Spectroscopic Evolution For A Representative Sample Of SNe Ibn The Spectra Are Reddening Corrected

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