P
Priscilla J. Benson
Researcher at Wellesley College
Publications - 31
Citations - 5668
Priscilla J. Benson is an academic researcher from Wellesley College. The author has contributed to research in topics: Stars & Star formation. The author has an hindex of 19, co-authored 31 publications receiving 5472 citations.
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Journal ArticleDOI
BVRI Light Curves for 22 Type Ia Supernovae
Adam G. Riess,Robert P. Kirshner,Brian P. Schmidt,Saurabh Jha,Peter Challis,Peter M. Garnavich,Ann A. Esin,Christopher L. Carpenter,Randy Grashius,Rudolph E. Schild,Perry Berlind,John P. Huchra,Charles F. Prosser,Emilio E. Falco,Priscilla J. Benson,Cesar Briceno,Warren R. Brown,Nelson Caldwell,Ian P. Dell'Antonio,Alexei V. Filippenko,Alyssa A. Goodman,Norman A. Grogin,Ted Groner,John P. Hughes,Paul J. Green,Rolf A. Jansen,Jan T. Kleyna,Jane Luu,Lucas M. Macri,Brian McLeod,Kim K. McLeod,Brian R. McNamara,Brian McLean,Alejandra A. E. Milone,Joseph J. Mohr,Dan Moraru,Chien Y. Peng,Chien Y. Peng,J. Peters,Andrea Prestwich,Krzysztof Z. Stanek,Andy Szentgyorgyi,Ping Zhao,Ping Zhao +43 more
TL;DR: In this article, Johnson/Cousins B, V, R, and I photometric observations of 22 recent Type Ia supernovae (SNe Ia): SNe 1993ac, 1993ae, 1994M, 1994S, 1994T, 1994Q, 1994ae, 1995D, 1995E, 1995al, 1995ac, 1995ak, 1995bd, 1996C, 1996X, 1996Z, 1996ab, 1996ai, 1996bk, 1996bl, 1996bo, and 1996bv.
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Dense cores in dark clouds. VIII - Velocity gradients
TL;DR: In this paper, an analysis of motions consistent with uniform rotation in dense cores is presented, and the specific angular momentum is found to scale roughly as F exp 3/2, where R represents the diameter of the FWHM intensity contour in a map.
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Dense Cores in Dark Clouds. XIV. N2H+ (1-0) Maps of Dense Cloud Cores
TL;DR: In this article, an extensive mapping survey of N2H+ (1-0) in about 60 low-mass cloud cores already mapped in the NH3 (1, 1) inversion transition line is presented.
Journal ArticleDOI
A survey for dense cores in dark clouds
TL;DR: In this paper, a total of 149 dark cloud positions were surveyed for evidence of dense cores in the (J,K) = (1,1) rotating inversion line of NH3.
Journal ArticleDOI
Dense Cores in Dark Clouds. XIV. N2H+(1-0) maps of dense cloud cores
TL;DR: In this paper, the authors present results of an extensive mapping survey of N2H+(1-0) in about 60 low mass cloud cores already mapped in the NH3(1,1) inversion transition line.