Black hole mass estimates based on C IV are consistent with those based on the 
Balmer lines

Assef, R. J.; Denney, K. D.; Kochanek, C. S.; Peterson, B. M.; Kozłowski, S.; Ageorges, N.; Barrows, R. S.; Buschkamp, P.; Dietrich, M.; Falco, E.; Feiz, C.; Gemperlein, H.; Germeroth, A.; Grier, C. J.; Hofmann, R.; Juette, M.; Khan, R.; Kilic, M.; Knierim, V.; Laun, W.; Lederer, R.; Lehmitz, M.; Lenzen, R.; Mall, U.; Madsen, K. K.; Mandel, H.; Martini, P.; Mathur, S.; Mogren, K.; Mueller, P.; Naranjo, V.; Pasquali, A.; Polsterer, K.; Pogge, R. W.; Quirrenbach, A.; Seifert, W.; Stern, D.; Shappee, B.; Storz, C.; Van Saders, J.; Weiser, P.; Zhang, D.

doi:10.1088/0004-637X/742/2/93

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Black hole mass estimates based on C IV are consistent with those based on the Balmer lines

MPS-Authors

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Ageorges, N.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons18580

Buschkamp, P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4915

Gemperlein, H.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4776

Hofmann, R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons18582

Lederer, R.
MPI for Extraterrestrial Physics, Max Planck Society;

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引用

Assef, R. J., Denney, K. D., Kochanek, C. S., Peterson, B. M., Kozłowski, S., Ageorges, N., Barrows, R. S., Buschkamp, P., Dietrich, M., Falco, E., Feiz, C., Gemperlein, H., Germeroth, A., Grier, C. J., Hofmann, R., Juette, M., Khan, R., Kilic, M., Knierim, V., Laun, W., Lederer, R., Lehmitz, M., Lenzen, R., Mall, U., Madsen, K. K., Mandel, H., Martini, P., Mathur, S., Mogren, K., Mueller, P., Naranjo, V., Pasquali, A., Polsterer, K., Pogge, R. W., Quirrenbach, A., Seifert, W., Stern, D., Shappee, B., Storz, C., Van Saders, J., Weiser, P., & Zhang, D. (2011). Black hole mass estimates based on C IV are consistent with those based on the Balmer lines. The Astrophysical Journal, 742(2):, pp. 1-26. doi:10.1088/0004-637X/742/2/93.

引用: https://hdl.handle.net/11858/00-001M-0000-000F-3A51-1

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