A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779

M. E. L. Hopwood; T. P. Roberts; M.R. Burleigh; M. Odenkirchen; A. P. Beardmore; P. T. O'Brien; R. D. Jeffries; A. J. Penny; S. P. S. Eyres; A. Evans

doi:10.1046/j.1365-8711.2000.03717.x

A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779

M. E. L. Hopwood, T. P. Roberts, M.R. Burleigh, M. Odenkirchen, A. P. Beardmore, P. T. O'Brien, R. D. Jeffries, A. J. Penny, S. P. S. Eyres, A. Evans

Cyfadran Cyfrifiadureg, Peirianneg a Gwyddoniaeth

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

Crynodeb

We report the possible detection of diffuse X-ray emission in the environment of NGC 6779, and find the emission to be well aligned with the proper motion of the cluster. The position of the emission suggests we are observing heated ISM in the wake of the cluster that could be the result of an interaction between the intracluster medium and the halo gas surrounding it.

Iaith wreiddiol	Saesneg
Tudalennau (o-i)	L5-L8
Cyfnodolyn	Monthly Notices of the Royal Astronomical Society
Cyfrol	316
Rhif cyhoeddi	1
Dynodwyr Gwrthrych Digidol (DOIs)	https://doi.org/10.1046/j.1365-8711.2000.03717.x
Statws	Cyhoeddwyd - 21 Gorff 2000

Mynediad at Ddogfen

10.1046/j.1365-8711.2000.03717.x

Dyfynnu hyn

Hopwood, M. E. L., Roberts, T. P., Burleigh, M. R., Odenkirchen, M., Beardmore, A. P., O'Brien, P. T., Jeffries, R. D., Penny, A. J., Eyres, S. P. S., & Evans, A. (2000). A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779. Monthly Notices of the Royal Astronomical Society, 316(1), L5-L8. https://doi.org/10.1046/j.1365-8711.2000.03717.x

@article{b2c9678aa1394e298cfa431e7ea8193d,

title = "A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779",

abstract = "We report the possible detection of diffuse X-ray emission in the environment of NGC 6779, and find the emission to be well aligned with the proper motion of the cluster. The position of the emission suggests we are observing heated ISM in the wake of the cluster that could be the result of an interaction between the intracluster medium and the halo gas surrounding it.",

keywords = "globular clusters : general, globular clusters: individual: NGC 6779, X-rays: ISM, X-rays: general",

author = "Hopwood, {M. E. L.} and Roberts, {T. P.} and M.R. Burleigh and M. Odenkirchen and Beardmore, {A. P.} and O'Brien, {P. T.} and Jeffries, {R. D.} and Penny, {A. J.} and Eyres, {S. P. S.} and A. Evans",

year = "2000",

month = jul,

day = "21",

doi = "10.1046/j.1365-8711.2000.03717.x",

language = "English",

volume = "316",

pages = "L5--L8",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Hopwood, MEL, Roberts, TP, Burleigh, MR, Odenkirchen, M, Beardmore, AP, O'Brien, PT, Jeffries, RD, Penny, AJ, Eyres, SPS & Evans, A 2000, 'A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779', Monthly Notices of the Royal Astronomical Society, cyfrol. 316, rhif 1, tt. L5-L8. https://doi.org/10.1046/j.1365-8711.2000.03717.x

TY - JOUR

T1 - A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779

AU - Hopwood, M. E. L.

AU - Roberts, T. P.

AU - Burleigh, M.R.

AU - Odenkirchen, M.

AU - Beardmore, A. P.

AU - O'Brien, P. T.

AU - Jeffries, R. D.

AU - Penny, A. J.

AU - Eyres, S. P. S.

AU - Evans, A.

PY - 2000/7/21

Y1 - 2000/7/21

N2 - We report the possible detection of diffuse X-ray emission in the environment of NGC 6779, and find the emission to be well aligned with the proper motion of the cluster. The position of the emission suggests we are observing heated ISM in the wake of the cluster that could be the result of an interaction between the intracluster medium and the halo gas surrounding it.

AB - We report the possible detection of diffuse X-ray emission in the environment of NGC 6779, and find the emission to be well aligned with the proper motion of the cluster. The position of the emission suggests we are observing heated ISM in the wake of the cluster that could be the result of an interaction between the intracluster medium and the halo gas surrounding it.

KW - globular clusters : general

KW - globular clusters: individual: NGC 6779

KW - X-rays: ISM

KW - X-rays: general

U2 - 10.1046/j.1365-8711.2000.03717.x

DO - 10.1046/j.1365-8711.2000.03717.x

M3 - Article

VL - 316

SP - L5-L8

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -

A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779

Crynodeb

Mynediad at Ddogfen

Ôl bys

Dyfynnu hyn