CDROM/AJ/V107/P1745 U, V, and I of M15 (Yanny+ 1994) ================================================================================ Globular Cluster Photometry with the Hubble Space Telescope. II. U, V, and I Measurements of M15 Brian Yanny, Puragra Guhathakurta, John N. Bahcall & Donald P. Schneider <1994, AJ, 107, 1745> =1994AJ....107.1745Y ================================================================================ Abstract: The projected density distribution of resolved stars near the center of M15 is shown to be consistent with either a power-law cusp N(r) ~ r^alpha, with alpha ~ -0.85 +/- 0.2, or with a King model with a core of radius <~ 2" (best fit r(core) = 1.3"). The inferred slope is in agreement with the theoretical value, alpha = -0.75, calculated by Bahcall and Wolf for the distribution of equal-mass stars surrounding a massive black hole and is also consistent with the radial profile expected from core collapse without a central black hole. The object AC 214 is a candidate for the central density cusp. Analysis of Monte Carlo simulations of the diffuse light indicates that, using current analysis techniques and available data, the residual light is not a reliable indicator of the true density distribution. This is contrary to earlier work. Photometric measurements in V and I of more than 5x10^3 stars (and in U, V, and I of >~ 1500 stars) are used to construct color-magnitude diagrams in the central 1' of M15. Fourteen blue straggler candidates are identified in the inner 20". The central color gradient noticed by previous researchers is caused by a central depletion of bright red giant stars rather than an excess of blue stragglers or blue horizontal branch stars. File Summary: -------------------------------------------------------------------------------- File Name Lrecl Records Explanations -------------------------------------------------------------------------------- table3.dat 37 1186 Stellar photometry and astrometry for M15 (V < 18.1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- ID Identification number 5-11 F7.2 arcsec RA *R.A. offset from AC 211 = ID 653 12-18 F7.2 arcsec DE *Dec. offset from AC 211 = ID 653 19-24 F6.2 mag V Visual magnitude 25-30 F6.2 mag V-I V-I color 31-36 F6.2 mag U-V []? U-V color 37 A1 --- n_U-V *[ab] Note for U-V -------------------------------------------------------------------------------- Notes for file: table3.dat -------------------------------------------------------------------------------- RA,DE: Coordinates are arcsec offsets relative to AC 211 = ID 653. ID 653 is at RA(2000)= 21:29:58.26 DEC(2000)=12:10:02.90 n_U-V: a - the star is located outside the area covered by the U image. b - the star is not detected in U, though the area was covered. -------------------------------------------------------------------------------- ================================================================================ (End) Lee Brotzman [ADS] 17-May-1994