Host galaxy magnitude of OJ 287 from its colours at minimum
light

J 2022

Host galaxy magnitude of OJ 287 from its colours at minimum light

VALTONEN, Mauri J.; Lankeswar DEY; Stanislaw ZOLA; S. CIPRINI; M. KIDGER et al.

Základní údaje

Originální název

Host galaxy magnitude of OJ 287 from its colours at minimum light

Autoři

VALTONEN, Mauri J.; Lankeswar DEY; Stanislaw ZOLA; S. CIPRINI; M. KIDGER; T. PURSIMO; A. GOPAKUMAR; K. MATSUMOTO; K. SADAKANE; D. B. CATON; K. NILSSON; S. KOMOSSA; M. BAGAGLIA; A. BARANSKY; P. BOUMIS; D. BOYD; A. J. CASTRO-TIRADO; B. DEBSKI; M. DROZDZ; A. E. PEREZE; M. FIORUCCI; F. GARCIA; K. GAZEAS; S. GHOSH; V. GODUNOVA; J. L. GOMEZ; R. GREDEL; D. GRUPE; J. B. HAISLIP; T. HENNING; G. HURST; Jan JANÍK ; V. V. KOUPRIANOV; H. LEHTO; A. LIAKOS; S. MATHUR; M. MUGRAUER; R. N. NOGUES; G. NUCCIARELLI; W. OGLOZA; D. K. OJHA; U. PAJDOSZ-SMIERCIAK; S. PASCOLINI; G. POYNER; D. E. REICHART; N. RIZZI; F. RONCELLA; D. K. SAHU; A. SILLANPAA; A. SIMON; M. SIWAK; F. C. SOLDAN ALFARO; E. SONBAS; G. TOSTI; V. VASYLENKO; J. R. WEBB a P. ZIELINSKI

Vydání

Monthly Notices of the Royal Astronomical Society, MALDEN, WILEY, 2022, 0035-8711

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Velká Británie a Severní Irsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

URL, URL

Impakt faktor

Impact factor: 4.800

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/22:00126442

Organizační jednotka

Přírodovědecká fakulta

Klíčová slova anglicky

galaxies: active; BL Lacertae objects: general; BL Lacertae objects: individual: OJ 287; galaxies: bulges

Štítky

14312040, rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 6. 12. 2022 11:09, Mgr. Marie Novosadová Šípková, DiS.

Anotace

V originále

OJ 287 is a BL Lacertae type quasar in which the active galactic nucleus (AGN) outshines the host galaxy by an order of magnitude. The only exception to this may be at minimum light when the AGN activity is so low that the host galaxy may make quite a considerable contribution to the photometric intensity of the source. Such a dip or a fade in the intensity of OJ 287 occurred in 2017 November, when its brightness was about 1.75 mag lower than the recent mean level. We compare the observations of this fade with similar fades in OJ 287 observed earlier in 1989, 1999, and 2010. It appears that there is a relatively strong reddening of the B- V colours of OJ 287 when its V-band brightness drops below magnitude 17. Similar changes are also seen in V- R, V- I, and R- I colours during these deep fades. These data support the conclusion that the total magnitude of the host galaxy is V = 18.0 +/- 0.3, corresponding to M-K = -26.5 +/- 0.3 in the K-band. This is in agreement with the results, obtained using the integrated surface brightness method, from recent surface photometry of the host. These results should encourage us to use the colour separation method also in other host galaxies with strongly variable AGN. In the case of OJ 287, both the host galaxy and its central black hole are among the biggest known, and its position in the black hole mass-galaxy mass diagram lies close to the mean correlation.

Citovat

VALTONEN, Mauri J.; Lankeswar DEY; Stanislaw ZOLA; S. CIPRINI; M. KIDGER; T. PURSIMO; A. GOPAKUMAR; K. MATSUMOTO; K. SADAKANE; D. B. CATON; K. NILSSON; S. KOMOSSA; M. BAGAGLIA; A. BARANSKY; P. BOUMIS; D. BOYD; A. J. CASTRO-TIRADO; B. DEBSKI; M. DROZDZ; A. E. PEREZE; M. FIORUCCI; F. GARCIA; K. GAZEAS; S. GHOSH; V. GODUNOVA; J. L. GOMEZ; R. GREDEL; D. GRUPE; J. B. HAISLIP; T. HENNING; G. HURST; Jan JANÍK; V. V. KOUPRIANOV; H. LEHTO; A. LIAKOS; S. MATHUR; M. MUGRAUER; R. N. NOGUES; G. NUCCIARELLI; W. OGLOZA; D. K. OJHA; U. PAJDOSZ-SMIERCIAK; S. PASCOLINI; G. POYNER; D. E. REICHART; N. RIZZI; F. RONCELLA; D. K. SAHU; A. SILLANPAA; A. SIMON; M. SIWAK; F. C. SOLDAN ALFARO; E. SONBAS; G. TOSTI; V. VASYLENKO; J. R. WEBB a P. ZIELINSKI. Host galaxy magnitude of OJ 287 from its colours at minimum light. Monthly Notices of the Royal Astronomical Society. MALDEN: WILEY, 2022, roč. 514, č. 2, s. 3017-3023. ISSN 0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stac1522.

@article{2211837,
   author = {Valtonen, Mauri J. and Dey, Lankeswar and Zola, Stanislaw and Ciprini, S. and Kidger, M. and Pursimo, T. and Gopakumar, A. and Matsumoto, K. and Sadakane, K. and Caton, D. B. and Nilsson, K. and Komossa, S. and Bagaglia, M. and Baransky, A. and Boumis, P. and Boyd, D. and CastroandTirado, A. J. and Debski, B. and Drozdz, M. and Pereze, A. E. and Fiorucci, M. and Garcia, F. and Gazeas, K. and Ghosh, S. and Godunova, V. and Gomez, J. L. and Gredel, R. and Grupe, D. and Haislip, J. B. and Henning, T. and Hurst, G. and Janík, Jan and Kouprianov, V. V. and Lehto, H. and Liakos, A. and Mathur, S. and Mugrauer, M. and Nogues, R. N. and Nucciarelli, G. and Ogloza, W. and Ojha, D. K. and PajdoszandSmierciak, U. and Pascolini, S. and Poyner, G. and Reichart, D. E. and Rizzi, N. and Roncella, F. and Sahu, D. K. and Sillanpaa, A. and Simon, A. and Siwak, M. and Soldan Alfaro, F. C. and Sonbas, E. and Tosti, G. and Vasylenko, V. and Webb, J. R. and Zielinski, P.},
   article_location = {MALDEN},
   article_number = {2},
   doi = {https://doi.org/10.1093/mnras/stac1522},
   keywords = {galaxies: active; BL Lacertae objects: general; BL Lacertae objects: individual: OJ 287; galaxies: bulges},
   language = {eng},
   issn = {0035-8711},
   journal = {Monthly Notices of the Royal Astronomical Society},
   title = {Host galaxy magnitude of OJ 287 from its colours at minimum light},
   url = {https://academic.oup.com/mnras/article-abstract/514/2/3017/6598825?redirectedFrom=fulltext},
   volume = {514},
   year = {2022}
}

TY  - JOUR
ID  - 2211837
AU  - Valtonen, Mauri J. - Dey, Lankeswar - Zola, Stanislaw - Ciprini, S. - Kidger, M. - Pursimo, T. - Gopakumar, A. - Matsumoto, K. - Sadakane, K. - Caton, D. B. - Nilsson, K. - Komossa, S. - Bagaglia, M. - Baransky, A. - Boumis, P. - Boyd, D. - Castro-Tirado, A. J. - Debski, B. - Drozdz, M. - Pereze, A. E. - Fiorucci, M. - Garcia, F. - Gazeas, K. - Ghosh, S. - Godunova, V. - Gomez, J. L. - Gredel, R. - Grupe, D. - Haislip, J. B. - Henning, T. - Hurst, G. - Janík, Jan - Kouprianov, V. V. - Lehto, H. - Liakos, A. - Mathur, S. - Mugrauer, M. - Nogues, R. N. - Nucciarelli, G. - Ogloza, W. - Ojha, D. K. - Pajdosz-Smierciak, U. - Pascolini, S. - Poyner, G. - Reichart, D. E. - Rizzi, N. - Roncella, F. - Sahu, D. K. - Sillanpaa, A. - Simon, A. - Siwak, M. - Soldan Alfaro, F. C. - Sonbas, E. - Tosti, G. - Vasylenko, V. - Webb, J. R. - Zielinski, P.
PY  - 2022
TI  - Host galaxy magnitude of OJ 287 from its colours at minimum light
JF  - Monthly Notices of the Royal Astronomical Society
VL  - 514
IS  - 2
SP  - 3017-3023
EP  - 3017-3023
PB  - WILEY
SN  - 00358711
KW  - galaxies: active
KW  - BL Lacertae objects: general
KW  - BL Lacertae objects: individual: OJ 287
KW  - galaxies: bulges
UR  - https://academic.oup.com/mnras/article-abstract/514/2/3017/6598825?redirectedFrom=fulltext
N2  - OJ 287 is a BL Lacertae type quasar in which the active galactic nucleus (AGN) outshines the host galaxy by an order of magnitude. The only exception to this may be at minimum light when the AGN activity is so low that the host galaxy may make quite a considerable contribution to the photometric intensity of the source. Such a dip or a fade in the intensity of OJ 287 occurred in 2017 November, when its brightness was about 1.75 mag lower than the recent mean level. We compare the observations of this fade with similar fades in OJ 287 observed earlier in 1989, 1999, and 2010. It appears that there is a relatively strong reddening of the B- V colours of OJ 287 when its V-band brightness drops below magnitude 17. Similar changes are also seen in V- R, V- I, and R- I colours during these deep fades. These data support the conclusion that the total magnitude of the host galaxy is V = 18.0 +/- 0.3, corresponding to M-K = -26.5 +/- 0.3 in the K-band. This is in agreement with the results, obtained using the integrated surface brightness method, from recent surface photometry of the host. These results should encourage us to use the colour separation method also in other host galaxies with strongly variable AGN. In the case of OJ 287, both the host galaxy and its central black hole are among the biggest known, and its position in the black hole mass-galaxy mass diagram lies close to the mean correlation.
ER  -

VALTONEN, Mauri J.; Lankeswar DEY; Stanislaw ZOLA; S. CIPRINI; M. KIDGER; T. PURSIMO; A. GOPAKUMAR; K. MATSUMOTO; K. SADAKANE; D. B. CATON; K. NILSSON; S. KOMOSSA; M. BAGAGLIA; A. BARANSKY; P. BOUMIS; D. BOYD; A. J. CASTRO-TIRADO; B. DEBSKI; M. DROZDZ; A. E. PEREZE; M. FIORUCCI; F. GARCIA; K. GAZEAS; S. GHOSH; V. GODUNOVA; J. L. GOMEZ; R. GREDEL; D. GRUPE; J. B. HAISLIP; T. HENNING; G. HURST; Jan JANÍK; V. V. KOUPRIANOV; H. LEHTO; A. LIAKOS; S. MATHUR; M. MUGRAUER; R. N. NOGUES; G. NUCCIARELLI; W. OGLOZA; D. K. OJHA; U. PAJDOSZ-SMIERCIAK; S. PASCOLINI; G. POYNER; D. E. REICHART; N. RIZZI; F. RONCELLA; D. K. SAHU; A. SILLANPAA; A. SIMON; M. SIWAK; F. C. SOLDAN ALFARO; E. SONBAS; G. TOSTI; V. VASYLENKO; J. R. WEBB a P. ZIELINSKI. Host galaxy magnitude of OJ 287 from its colours at minimum light. \textit{Monthly Notices of the Royal Astronomical Society}. MALDEN: WILEY, 2022, roč.~514, č.~2, s.~3017-3023. ISSN~0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stac1522.

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