Probing the nature of the unidentified TeV gamma-ray source HESS J0632+057 with Swift

Abraham David Falcone, J. Grube, J. Hinton, J. Holder, G. Maier, R. Mukherjee, J. Skilton, M. Stroh

Research output: Contribution to journalArticle

27 Citations (Scopus)

Abstract

New generation TeV gamma-ray telescopes have discovered many new sources, including several enigmatic unidentified TeV objects. HESS J0632+057 is a particularly interesting unidentified TeV source since: it is a point source, it has a possible hard-spectrum X-ray counterpart and a positionally consistent Be star, it has evidence of long-term very high energy gamma-ray flux variability, and it is postulated to be a newly detected TeV/X-ray binary. We have obtained Swift X-ray telescope observations of this source from MJD 54857 to 54965, in an attempt to ascertain its nature and to investigate the hypothesis that it is a previously unknown X-ray/TeV binary. Variability and spectral properties similar to those of the other three known X-ray/TeV binaries have been observed, with measured flux increases by factors of ∼3. X-ray variability is present on multiple timescales including days to months; however, no clear signature of periodicity is present on the timescales probed by these data. If binary modulation is present and dominating the measured variability, then the period of the orbit is likely to be ≥54days (half of this campaign), or it has a shorter period with a variable degree of flux modulation on successive high states. If the two high states measured to date are due to binary modulation, then the favored period is approximately 35-40 days. More observations are required to determine if this object is truly a binary system and to determine the extent that the measured variability is due to inter-orbit flaring effects or periodic binary modulation.

Original languageEnglish (US)
JournalAstrophysical Journal Letters
Volume708
Issue number1 PART 2
DOIs
StatePublished - Jan 1 2010

Fingerprint

modulation
x rays
timescale
orbits
gamma ray telescopes
point sources
periodicity
point source
periodic variations
signatures
gamma rays
telescopes
stars
energy
flaring
effect

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Falcone, Abraham David ; Grube, J. ; Hinton, J. ; Holder, J. ; Maier, G. ; Mukherjee, R. ; Skilton, J. ; Stroh, M. / Probing the nature of the unidentified TeV gamma-ray source HESS J0632+057 with Swift. In: Astrophysical Journal Letters. 2010 ; Vol. 708, No. 1 PART 2.
@article{356266b124ea40d4a4506a009fd8be93,
title = "Probing the nature of the unidentified TeV gamma-ray source HESS J0632+057 with Swift",
abstract = "New generation TeV gamma-ray telescopes have discovered many new sources, including several enigmatic unidentified TeV objects. HESS J0632+057 is a particularly interesting unidentified TeV source since: it is a point source, it has a possible hard-spectrum X-ray counterpart and a positionally consistent Be star, it has evidence of long-term very high energy gamma-ray flux variability, and it is postulated to be a newly detected TeV/X-ray binary. We have obtained Swift X-ray telescope observations of this source from MJD 54857 to 54965, in an attempt to ascertain its nature and to investigate the hypothesis that it is a previously unknown X-ray/TeV binary. Variability and spectral properties similar to those of the other three known X-ray/TeV binaries have been observed, with measured flux increases by factors of ∼3. X-ray variability is present on multiple timescales including days to months; however, no clear signature of periodicity is present on the timescales probed by these data. If binary modulation is present and dominating the measured variability, then the period of the orbit is likely to be ≥54days (half of this campaign), or it has a shorter period with a variable degree of flux modulation on successive high states. If the two high states measured to date are due to binary modulation, then the favored period is approximately 35-40 days. More observations are required to determine if this object is truly a binary system and to determine the extent that the measured variability is due to inter-orbit flaring effects or periodic binary modulation.",
author = "Falcone, {Abraham David} and J. Grube and J. Hinton and J. Holder and G. Maier and R. Mukherjee and J. Skilton and M. Stroh",
year = "2010",
month = "1",
day = "1",
doi = "10.1088/2041-8205/708/1/L52",
language = "English (US)",
volume = "708",
journal = "Astrophysical Journal Letters",
issn = "2041-8205",
publisher = "IOP Publishing Ltd.",
number = "1 PART 2",

}

Falcone, AD, Grube, J, Hinton, J, Holder, J, Maier, G, Mukherjee, R, Skilton, J & Stroh, M 2010, 'Probing the nature of the unidentified TeV gamma-ray source HESS J0632+057 with Swift', Astrophysical Journal Letters, vol. 708, no. 1 PART 2. https://doi.org/10.1088/2041-8205/708/1/L52

Probing the nature of the unidentified TeV gamma-ray source HESS J0632+057 with Swift. / Falcone, Abraham David; Grube, J.; Hinton, J.; Holder, J.; Maier, G.; Mukherjee, R.; Skilton, J.; Stroh, M.

In: Astrophysical Journal Letters, Vol. 708, No. 1 PART 2, 01.01.2010.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Probing the nature of the unidentified TeV gamma-ray source HESS J0632+057 with Swift

AU - Falcone, Abraham David

AU - Grube, J.

AU - Hinton, J.

AU - Holder, J.

AU - Maier, G.

AU - Mukherjee, R.

AU - Skilton, J.

AU - Stroh, M.

PY - 2010/1/1

Y1 - 2010/1/1

N2 - New generation TeV gamma-ray telescopes have discovered many new sources, including several enigmatic unidentified TeV objects. HESS J0632+057 is a particularly interesting unidentified TeV source since: it is a point source, it has a possible hard-spectrum X-ray counterpart and a positionally consistent Be star, it has evidence of long-term very high energy gamma-ray flux variability, and it is postulated to be a newly detected TeV/X-ray binary. We have obtained Swift X-ray telescope observations of this source from MJD 54857 to 54965, in an attempt to ascertain its nature and to investigate the hypothesis that it is a previously unknown X-ray/TeV binary. Variability and spectral properties similar to those of the other three known X-ray/TeV binaries have been observed, with measured flux increases by factors of ∼3. X-ray variability is present on multiple timescales including days to months; however, no clear signature of periodicity is present on the timescales probed by these data. If binary modulation is present and dominating the measured variability, then the period of the orbit is likely to be ≥54days (half of this campaign), or it has a shorter period with a variable degree of flux modulation on successive high states. If the two high states measured to date are due to binary modulation, then the favored period is approximately 35-40 days. More observations are required to determine if this object is truly a binary system and to determine the extent that the measured variability is due to inter-orbit flaring effects or periodic binary modulation.

AB - New generation TeV gamma-ray telescopes have discovered many new sources, including several enigmatic unidentified TeV objects. HESS J0632+057 is a particularly interesting unidentified TeV source since: it is a point source, it has a possible hard-spectrum X-ray counterpart and a positionally consistent Be star, it has evidence of long-term very high energy gamma-ray flux variability, and it is postulated to be a newly detected TeV/X-ray binary. We have obtained Swift X-ray telescope observations of this source from MJD 54857 to 54965, in an attempt to ascertain its nature and to investigate the hypothesis that it is a previously unknown X-ray/TeV binary. Variability and spectral properties similar to those of the other three known X-ray/TeV binaries have been observed, with measured flux increases by factors of ∼3. X-ray variability is present on multiple timescales including days to months; however, no clear signature of periodicity is present on the timescales probed by these data. If binary modulation is present and dominating the measured variability, then the period of the orbit is likely to be ≥54days (half of this campaign), or it has a shorter period with a variable degree of flux modulation on successive high states. If the two high states measured to date are due to binary modulation, then the favored period is approximately 35-40 days. More observations are required to determine if this object is truly a binary system and to determine the extent that the measured variability is due to inter-orbit flaring effects or periodic binary modulation.

UR - http://www.scopus.com/inward/record.url?scp=77949522696&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=77949522696&partnerID=8YFLogxK

U2 - 10.1088/2041-8205/708/1/L52

DO - 10.1088/2041-8205/708/1/L52

M3 - Article

AN - SCOPUS:77949522696

VL - 708

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

SN - 2041-8205

IS - 1 PART 2

ER -