S FIS 1002281 bibliography
51
DAFTAR PUSTAKA
Bahcall, J, N. (2000). “How The Sun Shines”. Nobel Foundation. Retrieved 200608-30.
Battaglini, F; P, P, Brollo; L, Cassarini & P, Sabbadin. (2010). “Photometric
Analysis of the Open Cluster Ngc 6791”. I1 Cielo come Laboratorio, 1.
Binney, J & Merrifeld, M. (1998). Galactic Astronomy. Princeton, New Jersey:
Princeton University Press.
de la Fuente Marcos. R. (1998). “Dynamical Evolution of Open Star Cluster”.
Publication of the Astronomical Society of the Pacific 110 (751): 1117-
1117.
Formert, H & K, Christine. (2007). “Open Star Cluster”. SEDS. University of
Arizona, Lunar and Planetary Lab. Retrieved 2009-01-02.
Hills, J, G. (1980). “The Offect of Mass Loss On The Dynamical Evolution of
Stellar System – Analitycal Approximations”. Astrophysical Journal
235: 986-991.
Howell, S, B. (2006). Handbook of CCD Astronomy. Cambridge: Cambridge
University Press.
Kroupa, P; S. Aarseth. & J. Hurley. (2001). “The Formation of a Bound Star
Cluster: from the Orion Nebula Cluster to the Pleiades”. Monthly Notices
of the Royal Astronomical Society 321 (4): 699-712.
Kroupa, P. (2004). “The Fundamental Building Blocks of Galaxy”. Procedings of
the Gaia Symposium “The Three-Dimensional Universe With Gaia”(ESA
SP-576). Observatoire de Paris-Meudon p.629. arXiv:astro-ph/0412069.
FAJAR RAMADHAN, 2015
FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)
Universitas Pendidikan Indonesia | repository.upi.edu | perpustakaan.upi.edu
52
Lada, C, J. (2010). “The Physics and Modes of Star Cluster Formation:
Observations”. Philosophical Transaction of the Royal Society A 368 :
713-731.
Montgomery, K, A; L, A, Marschall & K, A, Janes. (1993). “CCD Photometry of
the Old Open Cluster M67”. The Astronomical Journal Vol. 106: 181219.
Naim, S. O. & Evgeny, G. (2012). “Examining the M67 Classification as an Open
Cluster”. International Journal of Astrophysics, 2012, 2: 167-173.
Nilakshi, S. R; Pandey, A.K. & Mohan, V. (2002). “A study of spatial structure of
galactic open star clusters”. Astronomy and Astrophysics 383 (1): 153–
162
Payne-Gaposchkin, C. (1979). “Stars and Clusters”. Cambridge: Harvard
University Press.
Percival, S, M; Salaris, M. & Kilkenny, D. (2003). “The Open Cluster Distance
Scale – A New Empirical Approach”. Astronomy & Astrophysics 400:
541-552.
Sanders, W. L. (1977). “Membership of the Open Cluster M67”. Astronomy and
Astrophysics Supplement Series 27: 89-116
Sanders, W. L. (1989). “UBV Photometry of M67 Members”. Rev Mexicana
Astron. Astrof 17: 31-35.
Sarajedini, A; A, Dotter. & K, Allyson. (2009). “Deep 2MASS Photometry of
M67 and Calibration of the Main Sequence J-KS Color Difference as an
Age Indicator”. AJ , 2009.
Szebehely, V, G. & Curran, R, B. (1985). “Stability of the Solar System and Its
Minor Natural and Artificial Bodies”. Springer . ISBN 90-277-2046-0.
FAJAR RAMADHAN, 2015
FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)
Universitas Pendidikan Indonesia | repository.upi.edu | perpustakaan.upi.edu
53
Yakut, K; W, Zima; B, Kalomeni; H, van Wickel; C, Waelkens; P, De Cat; E,
Bauwens; M, Vuckovic; S, Saesen; L, Le Guillou; M, Parmaksizoglu; K,
Oluc; I, Khamitov; G, Raskin & C, Aerts. (2009). “Close Binary and
Other Variable Stars in the Solar Age Galactic Open Cluster M67”.
Astronomy and Astrophysics Vol. 505 : 165-176.
Brucegary.net/M67
http://dss.nao.ac.jp
stev.oapd.inaf.it
www.univie.ac.at/webda
FAJAR RAMADHAN, 2015
FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)
Universitas Pendidikan Indonesia | repository.upi.edu | perpustakaan.upi.edu
DAFTAR PUSTAKA
Bahcall, J, N. (2000). “How The Sun Shines”. Nobel Foundation. Retrieved 200608-30.
Battaglini, F; P, P, Brollo; L, Cassarini & P, Sabbadin. (2010). “Photometric
Analysis of the Open Cluster Ngc 6791”. I1 Cielo come Laboratorio, 1.
Binney, J & Merrifeld, M. (1998). Galactic Astronomy. Princeton, New Jersey:
Princeton University Press.
de la Fuente Marcos. R. (1998). “Dynamical Evolution of Open Star Cluster”.
Publication of the Astronomical Society of the Pacific 110 (751): 1117-
1117.
Formert, H & K, Christine. (2007). “Open Star Cluster”. SEDS. University of
Arizona, Lunar and Planetary Lab. Retrieved 2009-01-02.
Hills, J, G. (1980). “The Offect of Mass Loss On The Dynamical Evolution of
Stellar System – Analitycal Approximations”. Astrophysical Journal
235: 986-991.
Howell, S, B. (2006). Handbook of CCD Astronomy. Cambridge: Cambridge
University Press.
Kroupa, P; S. Aarseth. & J. Hurley. (2001). “The Formation of a Bound Star
Cluster: from the Orion Nebula Cluster to the Pleiades”. Monthly Notices
of the Royal Astronomical Society 321 (4): 699-712.
Kroupa, P. (2004). “The Fundamental Building Blocks of Galaxy”. Procedings of
the Gaia Symposium “The Three-Dimensional Universe With Gaia”(ESA
SP-576). Observatoire de Paris-Meudon p.629. arXiv:astro-ph/0412069.
FAJAR RAMADHAN, 2015
FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)
Universitas Pendidikan Indonesia | repository.upi.edu | perpustakaan.upi.edu
52
Lada, C, J. (2010). “The Physics and Modes of Star Cluster Formation:
Observations”. Philosophical Transaction of the Royal Society A 368 :
713-731.
Montgomery, K, A; L, A, Marschall & K, A, Janes. (1993). “CCD Photometry of
the Old Open Cluster M67”. The Astronomical Journal Vol. 106: 181219.
Naim, S. O. & Evgeny, G. (2012). “Examining the M67 Classification as an Open
Cluster”. International Journal of Astrophysics, 2012, 2: 167-173.
Nilakshi, S. R; Pandey, A.K. & Mohan, V. (2002). “A study of spatial structure of
galactic open star clusters”. Astronomy and Astrophysics 383 (1): 153–
162
Payne-Gaposchkin, C. (1979). “Stars and Clusters”. Cambridge: Harvard
University Press.
Percival, S, M; Salaris, M. & Kilkenny, D. (2003). “The Open Cluster Distance
Scale – A New Empirical Approach”. Astronomy & Astrophysics 400:
541-552.
Sanders, W. L. (1977). “Membership of the Open Cluster M67”. Astronomy and
Astrophysics Supplement Series 27: 89-116
Sanders, W. L. (1989). “UBV Photometry of M67 Members”. Rev Mexicana
Astron. Astrof 17: 31-35.
Sarajedini, A; A, Dotter. & K, Allyson. (2009). “Deep 2MASS Photometry of
M67 and Calibration of the Main Sequence J-KS Color Difference as an
Age Indicator”. AJ , 2009.
Szebehely, V, G. & Curran, R, B. (1985). “Stability of the Solar System and Its
Minor Natural and Artificial Bodies”. Springer . ISBN 90-277-2046-0.
FAJAR RAMADHAN, 2015
FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)
Universitas Pendidikan Indonesia | repository.upi.edu | perpustakaan.upi.edu
53
Yakut, K; W, Zima; B, Kalomeni; H, van Wickel; C, Waelkens; P, De Cat; E,
Bauwens; M, Vuckovic; S, Saesen; L, Le Guillou; M, Parmaksizoglu; K,
Oluc; I, Khamitov; G, Raskin & C, Aerts. (2009). “Close Binary and
Other Variable Stars in the Solar Age Galactic Open Cluster M67”.
Astronomy and Astrophysics Vol. 505 : 165-176.
Brucegary.net/M67
http://dss.nao.ac.jp
stev.oapd.inaf.it
www.univie.ac.at/webda
FAJAR RAMADHAN, 2015
FOTOMETRI GUGUS BINTANG TERBUKA M67 (NGC 2682)
Universitas Pendidikan Indonesia | repository.upi.edu | perpustakaan.upi.edu