Old-Aged Primary Distance Indicators

被引:67
作者
Beaton, Rachael L. [1 ,2 ]
Bono, Giuseppe [3 ,4 ]
Braga, Vittorio Francesco [3 ,5 ]
Dall'Ora, Massimo [6 ]
Fiorentino, Giuliana [7 ]
Jang, In Sung [8 ]
Martinez-Vazquez, Clara E. [9 ]
Matsunaga, Noriyuki [10 ]
Monelli, Matteo [11 ,12 ]
Neeley, Jillian R. [13 ]
Salaris, Maurizio [14 ]
机构
[1] Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA
[2] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA
[3] Univ Roma Tor Vergata, Dept Phys, Rome, Italy
[4] INAF, Osservatorio Astron Roma, Rome, Italy
[5] ASDC, Rome, Italy
[6] INAF, Osservatorio Astron Capodimonte, Naples, Italy
[7] INAF, OAS Osservatorio Astrofis & Sci Spazio Bologna, Bologna, Italy
[8] Leibniz Inst Astrophys Potsdam, D-14482 Potsdam, Germany
[9] Natl Opt Astron Observ, Cerro Tololo Interamer, Casilla 603, La Serena, Chile
[10] Univ Tokyo, Sch Sci, Dept Astron, Tokyo, Japan
[11] IAC, Calle Via Lactea S-N, Tenerife 38205, Spain
[12] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
[13] Florida Atlantic Univ, Dept Phys, 777 Glades Rd, Boca Raton, FL 33431 USA
[14] Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England
基金
日本学术振兴会;
关键词
Distance scale; Population II stars; RR Lyrae; Type II Cepheids; Tip of the red giant branch; Old stars; Standard candles; Variable stars; RR-LYRAE STARS; RED GIANT BRANCH; LARGE-MAGELLANIC-CLOUD; PERIOD-LUMINOSITY RELATION; GALACTIC GLOBULAR-CLUSTERS; NEAR-INFRARED PHOTOMETRY; RV-TAURI STARS; CEPHEID PULSATION MODELS; BAADE-WESSELINK METHOD; GRAVITATIONAL LENSING EXPERIMENT;
D O I
10.1007/s11214-018-0542-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Old-aged stellar distance indicators are present in all Galactic structures (halo, bulge, disk) and in galaxies of all Hubble types and, thus, are immensely powerful tools for understanding our Universe. Here we present a comprehensive review for three primary standard candles from Population II: (i)RR Lyrae type variables (RRL), (ii)type II Cepheid variables (T2C), and (iii)the tip of the red giant branch (TRGB). The discovery and use of these distance indicators is placed in historical context before describing their theoretical foundations and demonstrating their observational applications across multiple wavelengths. The methods used to establish the absolute scale for each standard candle is described with a discussion of the observational systematics. We conclude by looking forward to the suite of new observational facilities anticipated over the next decade; these have both a broader wavelength coverage and larger apertures than current facilities. We anticipate future advancements in our theoretical understanding and observational application of these stellar populations as they apply to the Galactic and extragalactic distance scale.
引用
收藏
页数:93
相关论文
共 421 条
[1]   Some spectral criteria for the determination of absolute stellar magnitudes [J].
Adams, WS ;
Kohlschutter, A .
ASTROPHYSICAL JOURNAL, 1914, 40 (04) :385-398
[3]   The MACHO project LMC variable star inventory. VII. The discovery of RV Tauri stars and new type II Cepheids in the large magellanic cloud [J].
Alcock, C ;
Allsman, RA ;
Alves, DR ;
Axelrod, TS ;
Becker, A ;
Bennett, DP ;
Cook, KH ;
Freeman, KC ;
Griest, K ;
Lawson, WA ;
Lehner, MJ ;
Marshall, SL ;
Minniti, D ;
Peterson, BA ;
Pollard, KR ;
Pratt, MR ;
Quinn, PJ ;
Rodgers, AW ;
Sutherland, W ;
Tomaney, A ;
Welch, DL .
ASTRONOMICAL JOURNAL, 1998, 115 (05) :1921-1933
[4]   The Relationship of Sodium and Oxygen in Galactic Field RR Lyrae Stars [J].
Andrievsky, S. ;
Wallerstein, G. ;
Korotin, S. ;
Lyashko, D. ;
Kovtyukh, V. ;
Tsymbal, V. ;
Davis, C. E. ;
Gomez, T. ;
Huang, W. ;
Farrell, E. M. .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2018, 130 (984)
[5]  
[Anonymous], 2017, ARXIV170908079
[6]  
[Anonymous], 2016, GLASS UNIVERSE LADIE
[7]  
[Anonymous], 1958, RICERCHE ASTRONOMICH
[8]  
[Anonymous], 1975, EXTRAGALACTIC DISTAN
[9]  
[Anonymous], 2016, AA, DOI DOI 10.1051/0004-6361/201628714
[10]   Variable stars in nearby galaxies VII.: P-L relation in the BVRI bands of Cepheids in IC 1613 [J].
Antonello, E ;
Fossati, L ;
Fugazza, D ;
Mantegazza, L ;
Gieren, W .
ASTRONOMY & ASTROPHYSICS, 2006, 445 (03) :901-906