... 1996, ApJS, 106, 65 Merck, M., et al. 1995, IAU Colloq. ...
54. http://www.stsci.edu/~stefano/newcal97/pdf/aindex.pdf
... Heap, S., 84, 94, 114 Heyer, I., 398 Hill, R., 94, 106, 120 Hines, D., 217 Hodge, P., 47 Hook, R., 192, 518 Hulbert, S., 47, 52, 138 Jedrzejewski, R., 405, 413 Jefferys, W., 472 Joseph, C., 126 Kaiser, M., 29 Katsanis, R., 39 Keyes, C., 420, 440 Kimble, R ...
55. http://www.stsci.edu/~tle/papers/xrayemission_7469.pdf
... Welsh, W. F., Peterson, B. M., Koratkar, A. P., & Korista, K. T. 1998, ApJ, 509, 118 White, R. J., & Peterson, B. M. 1994, PASP, 106, 879 Yaqoob, T., & Warwick, R. S. 1991, MNRAS, 248, 773 Zdziarski, A. A., Johnson, W. N., & Magdziarz, P. 1996, MNRAS, 283 ...
56. http://www.stsci.edu/jwst/overview/history/drm/drm6.pdf
... Sequence of blue ob jects represents a star-formation rate of 2 M yr,1 for 106 years at z = 5, 10, 20 for an H0 = 50 =0:2, = 0 ...
57. http://www.stsci.edu/~inr/nstarpap/paper8.ps
... Heathcote, S. R., Walker, A. R., Gigoux, P., & Phillips, M. M. 1994, PASP, 106, 566 Harrington, R. S. & Dahn, C. C. 1980, AJ ...
58. The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I. Global
... wavelengths, three arc-like structures extending out to ~21, ~26 and ~31 kpc respectively, in the south-western part of M 31 ... The presence of these features, hosting ~2.2 У? 106 Mт?? of dust, is safely confirmed by their detection in HI maps. ...
59. http://www.stsci.edu/~stefano/newcal97/pdf/toc.pdf
... T. R. Gull, M. J. Taylor, R. Shaw, R. Robinson, and R. S. Hill 106 vi Contents 114 120 126 132 138 144 150 156 S. R. Heap and T. M. Brown Correction for the STIS Echelle Blaze Function . ...
60. The rarity of dust in metal-poor galaxies
... Draine, Bruce T., Donaldson, Jessica, Walter, Fabian, Sandstrom, Karin M., Leroy, Adam K., Cannon, John, & Gordon, Karl ... the Big Bang--is forming stars at a rate of 30-100 solar masses per year, yielding a mass assembly time of about 150ц—106 years ...