HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae

F. Aharonian; A. G. Akhperjanian; G. Anton; U. Barres De Almeida; A. R. Bazer-Bachi; Y. Becherini; B. Behera; K. Bernlöhr; C. Boisson; A. Bochow; V. Borrel; I. Braun; E. Brion; J. Brucker; P. Brun; R. Bühler; T. Bulik; I. Büsching; T. Boutelier; P. M. Chadwick; A. Charbonnier; R. V.G. Chaves; A. Cheesebrough; L. M. Chounet; A. C. Clapson; G. Coignet; M. Dalton; M. K. Daniel; I. D. Davids; B. Degrange; C. Deil; H. J. Dickinson; A. Djannati-Ataï; W. Domainko; L. Oc Drury; F. Dubois; G. Dubus; J. Dyks; M. Dyrda; K. Dgberts; D. Emmanoulopoulos; P. Espigat; C. Farnier; F. Feinstein; A. Fiasson; A. Förster; G. Fontaine; M. Füßling; S. Gabici; Y. A. Gallant; L. Gérard; B. Giebels; J. F. Glicenstein; B. Glück; P. Goret; D. Hauser; M. Hauser; S. Heinz; G. Heinzelmann; G. Henri; G. Hermann; J. A. Hinton; A. Hoffmann; W. Hofmann; M. Holleran; S. Hoppe; D. Horns; A. Jacholkowska; O. C. Fe jager; I. Jung; K. Katarzyński; U. Katz; S. Kaufmann; E. Kendziorra; M. Kerschhaggl; D. Khangulyan; B. Khélifi; D. Keogh; N. Nu Komin; K. Kosack; G. Lamanna; J. P. Lenain; T. Lohse; V. Marandon; J. M. Martin; O. Martineau-Huynh; A. Marcowith; D. Maurin; T. J.L. Mccomb; M. C. Medina; R. Moderski; E. Moulin; M. Naumann-Godo; M. De Naurois; D. Nedbal; D. Nekrassov; J. Niemiec; S. J. Nolan; S. Ohm; J. F. Olive; E. De Oña Wilhelmi; K. J. Orford; M. Ostrowski; M. Panter; M. Paz Arribas; G. Pedaletti; G. Pelletier; P. O. Petrucci; S. Pita; G. Pühlhofer; M. Punch; A. Quirrenbach; B. C. Raubenheimer; M. Raue; S. M. Rayner; O. Reimer; M. Renaud; F. Rieger; J. Ripken; L. Rob; S. Rosier-Lees; G. Rowell; B. Rudak; C. B. Rulten; J. Ruppel; V. Sahakian; A. Santangelo; R. Schlickeiser; F. M. Schöck; R. Schröder; U. Schwanke; S. Schwarzburg; S. Schwemmer; A. Shalchi; J. L. Skilton; H. Sol; D. Spangler; A. Stawarz; R. Steenkamp; C. Stegmann; G. Superina; A. Szostek; P. H. Tam; J. P. Tavernet; R. Terrier; O. Tibolla; C. Van eldik; G. Vasileiadis; C. Venter; L. Venter; J. P. Vialle; P. Vincent; M. Vivier; H. J. Völk; F. Volpe; S. J. Wagner; M. Ward; A. A. Zdziarski; A. Zech

doi:10.1051/0004-6361/200811564

HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae

F. Aharonian
, A. G. Akhperjanian
, G. Anton
, U. Barres De Almeida
, A. R. Bazer-Bachi
, Y. Becherini
, B. Behera
, K. Bernlöhr
, C. Boisson
, A. Bochow
, V. Borrel
, I. Braun
, E. Brion
, J. Brucker
, P. Brun
, R. Bühler
, T. Bulik
, I. Büsching
, T. Boutelier
, P. M. Chadwick

A. Charbonnier, R. V.G. Chaves, A. Cheesebrough, L. M. Chounet, A. C. Clapson, G. Coignet, M. Dalton, M. K. Daniel, I. D. Davids, B. Degrange, C. Deil, H. J. Dickinson, A. Djannati-Ataï, W. Domainko, L. Oc Drury, F. Dubois, G. Dubus, J. Dyks, M. Dyrda, K. Dgberts, D. Emmanoulopoulos, P. Espigat, C. Farnier, F. Feinstein, A. Fiasson, A. Förster, G. Fontaine, M. Füßling, S. Gabici, Y. A. Gallant, L. Gérard, B. Giebels, J. F. Glicenstein, B. Glück, P. Goret, D. Hauser, M. Hauser, S. Heinz, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, A. Hoffmann, W. Hofmann, M. Holleran, S. Hoppe, D. Horns, A. Jacholkowska, O. C. Fe jager, I. Jung, K. Katarzyński, U. Katz, S. Kaufmann, E. Kendziorra, M. Kerschhaggl, D. Khangulyan, B. Khélifi, D. Keogh, N. Nu Komin, K. Kosack, G. Lamanna, J. P. Lenain, T. Lohse, V. Marandon, J. M. Martin, O. Martineau-Huynh, A. Marcowith, D. Maurin, T. J.L. Mccomb, M. C. Medina, R. Moderski, E. Moulin, M. Naumann-Godo, M. De Naurois, D. Nedbal, D. Nekrassov, J. Niemiec, S. J. Nolan, S. Ohm, J. F. Olive, E. De Oña Wilhelmi, K. J. Orford, M. Ostrowski, M. Panter, M. Paz Arribas, G. Pedaletti, G. Pelletier, P. O. Petrucci, S. Pita, G. Pühlhofer, M. Punch, A. Quirrenbach, B. C. Raubenheimer, M. Raue, S. M. Rayner, O. Reimer, M. Renaud, F. Rieger, J. Ripken, L. Rob, S. Rosier-Lees, G. Rowell, B. Rudak, C. B. Rulten, J. Ruppel, V. Sahakian, A. Santangelo, R. Schlickeiser, F. M. Schöck, R. Schröder, U. Schwanke, S. Schwarzburg, S. Schwemmer, A. Shalchi, J. L. Skilton, H. Sol, D. Spangler, A. Stawarz, R. Steenkamp, C. Stegmann, G. Superina, A. Szostek, P. H. Tam, J. P. Tavernet, R. Terrier, O. Tibolla, C. Van eldik, G. Vasileiadis, C. Venter, L. Venter, J. P. Vialle, P. Vincent, M. Vivier, H. J. Völk, F. Volpe, S. J. Wagner, M. Ward, A. A. Zdziarski, A. Zech

Research output: Contribution to journal › Article › peer-review

Abstract

Observations of the globular cluster 47 Tucanae (NGC 104), which contains at least 23 ms pulsars, were performed with the HESS telescope system. The observations lead to an upper limit of F(E < 800 GeV) < 6.7 × 10-13 cm-2 s-1 on the integral γ-ray photon flux from 47 Tucanae. Considering millisecond pulsars as the unique potential source of γ-rays in the globular cluster, constraints based on emission models are derived: on the magnetic field in the average pulsar nebula and on the conversion efficiency of spin-down power to γ-ray photons or to relativistic leptons.

Original language	English
Pages (from-to)	273-277
Number of pages	5
Journal	Astronomy and Astrophysics
Volume	499
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361/200811564
Publication status	Published - 1 May 2009
Externally published	Yes

Keywords

Galaxy: globular clusters: individual: 47 Tucanae
Gamma rays: observations
Stars: pulsars: general

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10.1051/0004-6361/200811564

Cite this

Aharonian, F., Akhperjanian, A. G., Anton, G., Barres De Almeida, U., Bazer-Bachi, A. R., Becherini, Y., Behera, B., Bernlöhr, K., Boisson, C., Bochow, A., Borrel, V., Braun, I., Brion, E., Brucker, J., Brun, P., Bühler, R., Bulik, T., Büsching, I., Boutelier, T., ... Zech, A. (2009). HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae. Astronomy and Astrophysics, 499(1), 273-277. https://doi.org/10.1051/0004-6361/200811564

@article{a394596e7a8641af9d65f6410a78473f,

title = "HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae",

abstract = "Observations of the globular cluster 47 Tucanae (NGC 104), which contains at least 23 ms pulsars, were performed with the HESS telescope system. The observations lead to an upper limit of F(E < 800 GeV) < 6.7 × 10-13 cm-2 s-1 on the integral γ-ray photon flux from 47 Tucanae. Considering millisecond pulsars as the unique potential source of γ-rays in the globular cluster, constraints based on emission models are derived: on the magnetic field in the average pulsar nebula and on the conversion efficiency of spin-down power to γ-ray photons or to relativistic leptons.",

keywords = "Galaxy: globular clusters: individual: 47 Tucanae, Gamma rays: observations, Stars: pulsars: general",

author = "F. Aharonian and Akhperjanian, \{A. G.\} and G. Anton and \{Barres De Almeida\}, U. and Bazer-Bachi, \{A. R.\} and Y. Becherini and B. Behera and K. Bernl{\"o}hr and C. Boisson and A. Bochow and V. Borrel and I. Braun and E. Brion and J. Brucker and P. Brun and R. B{\"u}hler and T. Bulik and I. B{\"u}sching and T. Boutelier and Chadwick, \{P. M.\} and A. Charbonnier and Chaves, \{R. V.G.\} and A. Cheesebrough and Chounet, \{L. M.\} and Clapson, \{A. C.\} and G. Coignet and M. Dalton and Daniel, \{M. K.\} and Davids, \{I. D.\} and B. Degrange and C. Deil and Dickinson, \{H. J.\} and A. Djannati-Ata{\"i} and W. Domainko and Drury, \{L. Oc\} and F. Dubois and G. Dubus and J. Dyks and M. Dyrda and K. Dgberts and D. Emmanoulopoulos and P. Espigat and C. Farnier and F. Feinstein and A. Fiasson and A. F{\"o}rster and G. Fontaine and M. F{\"u}{\ss}ling and S. Gabici and Gallant, \{Y. A.\} and L. G{\'e}rard and B. Giebels and Glicenstein, \{J. F.\} and B. Gl{\"u}ck and P. Goret and D. Hauser and M. Hauser and S. Heinz and G. Heinzelmann and G. Henri and G. Hermann and Hinton, \{J. A.\} and A. Hoffmann and W. Hofmann and M. Holleran and S. Hoppe and D. Horns and A. Jacholkowska and \{Fe jager\}, \{O. C.\} and I. Jung and K. Katarzy{\'n}ski and U. Katz and S. Kaufmann and E. Kendziorra and M. Kerschhaggl and D. Khangulyan and B. Kh{\'e}lifi and D. Keogh and Komin, \{N. Nu\} and K. Kosack and G. Lamanna and Lenain, \{J. P.\} and T. Lohse and V. Marandon and Martin, \{J. M.\} and O. Martineau-Huynh and A. Marcowith and D. Maurin and Mccomb, \{T. J.L.\} and Medina, \{M. C.\} and R. Moderski and E. Moulin and M. Naumann-Godo and \{De Naurois\}, M. and D. Nedbal and D. Nekrassov and J. Niemiec and Nolan, \{S. J.\} and S. Ohm and Olive, \{J. F.\} and \{De O{\~n}a Wilhelmi\}, E. and Orford, \{K. J.\} and M. Ostrowski and M. Panter and \{Paz Arribas\}, M. and G. Pedaletti and G. Pelletier and Petrucci, \{P. O.\} and S. Pita and G. P{\"u}hlhofer and M. Punch and A. Quirrenbach and Raubenheimer, \{B. C.\} and M. Raue and Rayner, \{S. M.\} and O. Reimer and M. Renaud and F. Rieger and J. Ripken and L. Rob and S. Rosier-Lees and G. Rowell and B. Rudak and Rulten, \{C. B.\} and J. Ruppel and V. Sahakian and A. Santangelo and R. Schlickeiser and Sch{\"o}ck, \{F. M.\} and R. Schr{\"o}der and U. Schwanke and S. Schwarzburg and S. Schwemmer and A. Shalchi and Skilton, \{J. L.\} and H. Sol and D. Spangler and A. Stawarz and R. Steenkamp and C. Stegmann and G. Superina and A. Szostek and Tam, \{P. H.\} and Tavernet, \{J. P.\} and R. Terrier and O. Tibolla and \{Van eldik\}, C. and G. Vasileiadis and C. Venter and L. Venter and Vialle, \{J. P.\} and P. Vincent and M. Vivier and V{\"o}lk, \{H. J.\} and F. Volpe and Wagner, \{S. J.\} and M. Ward and Zdziarski, \{A. A.\} and A. Zech",

year = "2009",

month = may,

day = "1",

doi = "10.1051/0004-6361/200811564",

language = "English",

volume = "499",

pages = "273--277",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

number = "1",

}

Aharonian, F, Akhperjanian, AG, Anton, G, Barres De Almeida, U, Bazer-Bachi, AR, Becherini, Y, Behera, B, Bernlöhr, K, Boisson, C, Bochow, A, Borrel, V, Braun, I, Brion, E, Brucker, J, Brun, P, Bühler, R, Bulik, T, Büsching, I, Boutelier, T, Chadwick, PM, Charbonnier, A, Chaves, RVG, Cheesebrough, A, Chounet, LM, Clapson, AC, Coignet, G, Dalton, M, Daniel, MK, Davids, ID, Degrange, B, Deil, C, Dickinson, HJ, Djannati-Ataï, A, Domainko, W, Drury, LO, Dubois, F, Dubus, G, Dyks, J, Dyrda, M, Dgberts, K, Emmanoulopoulos, D, Espigat, P, Farnier, C, Feinstein, F, Fiasson, A, Förster, A, Fontaine, G, Füßling, M, Gabici, S, Gallant, YA, Gérard, L, Giebels, B, Glicenstein, JF, Glück, B, Goret, P, Hauser, D, Hauser, M, Heinz, S, Heinzelmann, G, Henri, G, Hermann, G, Hinton, JA, Hoffmann, A, Hofmann, W, Holleran, M, Hoppe, S, Horns, D, Jacholkowska, A, Fe jager, OC, Jung, I, Katarzyński, K, Katz, U, Kaufmann, S, Kendziorra, E, Kerschhaggl, M, Khangulyan, D, Khélifi, B, Keogh, D, Komin, NN, Kosack, K, Lamanna, G, Lenain, JP, Lohse, T, Marandon, V, Martin, JM, Martineau-Huynh, O, Marcowith, A, Maurin, D, Mccomb, TJL, Medina, MC, Moderski, R, Moulin, E, Naumann-Godo, M, De Naurois, M, Nedbal, D, Nekrassov, D, Niemiec, J, Nolan, SJ, Ohm, S, Olive, JF, De Oña Wilhelmi, E, Orford, KJ, Ostrowski, M, Panter, M, Paz Arribas, M, Pedaletti, G, Pelletier, G, Petrucci, PO, Pita, S, Pühlhofer, G, Punch, M, Quirrenbach, A, Raubenheimer, BC, Raue, M, Rayner, SM, Reimer, O, Renaud, M, Rieger, F, Ripken, J, Rob, L, Rosier-Lees, S, Rowell, G, Rudak, B, Rulten, CB, Ruppel, J, Sahakian, V, Santangelo, A, Schlickeiser, R, Schöck, FM, Schröder, R, Schwanke, U, Schwarzburg, S, Schwemmer, S, Shalchi, A, Skilton, JL, Sol, H, Spangler, D, Stawarz, A, Steenkamp, R, Stegmann, C, Superina, G, Szostek, A, Tam, PH, Tavernet, JP, Terrier, R, Tibolla, O, Van eldik, C, Vasileiadis, G, Venter, C, Venter, L, Vialle, JP, Vincent, P, Vivier, M, Völk, HJ, Volpe, F, Wagner, SJ, Ward, M, Zdziarski, AA & Zech, A 2009, 'HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae', Astronomy and Astrophysics, vol. 499, no. 1, pp. 273-277. https://doi.org/10.1051/0004-6361/200811564

TY - JOUR

T1 - HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae

AU - Aharonian, F.

AU - Akhperjanian, A. G.

AU - Anton, G.

AU - Barres De Almeida, U.

AU - Bazer-Bachi, A. R.

AU - Becherini, Y.

AU - Behera, B.

AU - Bernlöhr, K.

AU - Boisson, C.

AU - Bochow, A.

AU - Borrel, V.

AU - Braun, I.

AU - Brion, E.

AU - Brucker, J.

AU - Brun, P.

AU - Bühler, R.

AU - Bulik, T.

AU - Büsching, I.

AU - Boutelier, T.

AU - Chadwick, P. M.

AU - Charbonnier, A.

AU - Chaves, R. V.G.

AU - Cheesebrough, A.

AU - Chounet, L. M.

AU - Clapson, A. C.

AU - Coignet, G.

AU - Dalton, M.

AU - Daniel, M. K.

AU - Davids, I. D.

AU - Degrange, B.

AU - Deil, C.

AU - Dickinson, H. J.

AU - Djannati-Ataï, A.

AU - Domainko, W.

AU - Drury, L. Oc

AU - Dubois, F.

AU - Dubus, G.

AU - Dyks, J.

AU - Dyrda, M.

AU - Dgberts, K.

AU - Emmanoulopoulos, D.

AU - Espigat, P.

AU - Farnier, C.

AU - Feinstein, F.

AU - Fiasson, A.

AU - Förster, A.

AU - Fontaine, G.

AU - Füßling, M.

AU - Gabici, S.

AU - Gallant, Y. A.

AU - Gérard, L.

AU - Giebels, B.

AU - Glicenstein, J. F.

AU - Glück, B.

AU - Goret, P.

AU - Hauser, D.

AU - Hauser, M.

AU - Heinz, S.

AU - Heinzelmann, G.

AU - Henri, G.

AU - Hermann, G.

AU - Hinton, J. A.

AU - Hoffmann, A.

AU - Hofmann, W.

AU - Holleran, M.

AU - Hoppe, S.

AU - Horns, D.

AU - Jacholkowska, A.

AU - Fe jager, O. C.

AU - Jung, I.

AU - Katarzyński, K.

AU - Katz, U.

AU - Kaufmann, S.

AU - Kendziorra, E.

AU - Kerschhaggl, M.

AU - Khangulyan, D.

AU - Khélifi, B.

AU - Keogh, D.

AU - Komin, N. Nu

AU - Kosack, K.

AU - Lamanna, G.

AU - Lenain, J. P.

AU - Lohse, T.

AU - Marandon, V.

AU - Martin, J. M.

AU - Martineau-Huynh, O.

AU - Marcowith, A.

AU - Maurin, D.

AU - Mccomb, T. J.L.

AU - Medina, M. C.

AU - Moderski, R.

AU - Moulin, E.

AU - Naumann-Godo, M.

AU - De Naurois, M.

AU - Nedbal, D.

AU - Nekrassov, D.

AU - Niemiec, J.

AU - Nolan, S. J.

AU - Ohm, S.

AU - Olive, J. F.

AU - De Oña Wilhelmi, E.

AU - Orford, K. J.

AU - Ostrowski, M.

AU - Panter, M.

AU - Paz Arribas, M.

AU - Pedaletti, G.

AU - Pelletier, G.

AU - Petrucci, P. O.

AU - Pita, S.

AU - Pühlhofer, G.

AU - Punch, M.

AU - Quirrenbach, A.

AU - Raubenheimer, B. C.

AU - Raue, M.

AU - Rayner, S. M.

AU - Reimer, O.

AU - Renaud, M.

AU - Rieger, F.

AU - Ripken, J.

AU - Rob, L.

AU - Rosier-Lees, S.

AU - Rowell, G.

AU - Rudak, B.

AU - Rulten, C. B.

AU - Ruppel, J.

AU - Sahakian, V.

AU - Santangelo, A.

AU - Schlickeiser, R.

AU - Schöck, F. M.

AU - Schröder, R.

AU - Schwanke, U.

AU - Schwarzburg, S.

AU - Schwemmer, S.

AU - Shalchi, A.

AU - Skilton, J. L.

AU - Sol, H.

AU - Spangler, D.

AU - Stawarz, A.

AU - Steenkamp, R.

AU - Stegmann, C.

AU - Superina, G.

AU - Szostek, A.

AU - Tam, P. H.

AU - Tavernet, J. P.

AU - Terrier, R.

AU - Tibolla, O.

AU - Van eldik, C.

AU - Vasileiadis, G.

AU - Venter, C.

AU - Venter, L.

AU - Vialle, J. P.

AU - Vincent, P.

AU - Vivier, M.

AU - Völk, H. J.

AU - Volpe, F.

AU - Wagner, S. J.

AU - Ward, M.

AU - Zdziarski, A. A.

AU - Zech, A.

PY - 2009/5/1

Y1 - 2009/5/1

N2 - Observations of the globular cluster 47 Tucanae (NGC 104), which contains at least 23 ms pulsars, were performed with the HESS telescope system. The observations lead to an upper limit of F(E < 800 GeV) < 6.7 × 10-13 cm-2 s-1 on the integral γ-ray photon flux from 47 Tucanae. Considering millisecond pulsars as the unique potential source of γ-rays in the globular cluster, constraints based on emission models are derived: on the magnetic field in the average pulsar nebula and on the conversion efficiency of spin-down power to γ-ray photons or to relativistic leptons.

AB - Observations of the globular cluster 47 Tucanae (NGC 104), which contains at least 23 ms pulsars, were performed with the HESS telescope system. The observations lead to an upper limit of F(E < 800 GeV) < 6.7 × 10-13 cm-2 s-1 on the integral γ-ray photon flux from 47 Tucanae. Considering millisecond pulsars as the unique potential source of γ-rays in the globular cluster, constraints based on emission models are derived: on the magnetic field in the average pulsar nebula and on the conversion efficiency of spin-down power to γ-ray photons or to relativistic leptons.

KW - Galaxy: globular clusters: individual: 47 Tucanae

KW - Gamma rays: observations

KW - Stars: pulsars: general

UR - https://www.scopus.com/pages/publications/66349118357

U2 - 10.1051/0004-6361/200811564

DO - 10.1051/0004-6361/200811564

M3 - Article

AN - SCOPUS:66349118357

SN - 0004-6361

VL - 499

SP - 273

EP - 277

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 1

ER -

HESS upper limit on the very high energy γ-ray emission from the globular cluster 47 Tucanae

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Keywords

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