Open AccessConsequences of [ITAL]H[/ITAL][TINF]0[/TINF] = 69 ± 8 km s[TSUP]−1[/TSUP] Mpc[TSUP]−1[/TSUP] from Cepheid Variables in the Leo I Group
Author(s) -
Naoki Yasuda,
Sadanori Okamura
Publication year - 1996
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310269
Subject(s) - cepheid variable , physics , virgo cluster , astrophysics , surface brightness , tully–fisher relation , luminosity , astronomy , galaxy , stars , galaxy formation and evolution , galaxy cluster , galaxy rotation curve
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom