The Zeldovich Universe: Genesis and Growth of the Cosmic Web

Burcu Beygu; Kathryn Kreckel; Thijs van der Hulst; Reynier Peletier; Tom Jarrett; R. van de Weygaert; Jacqueline H. van Gorkom; Miguel Aragón-Calvo; R. van de Weygaert

doi:10.1017/S1743921316010656

The Zeldovich Universe: Genesis and Growth of the Cosmic Web

Burcu Beygu^*, Kathryn Kreckel, Thijs van der Hulst, Reynier Peletier, Tom Jarrett, R. van de Weygaert, Jacqueline H. van Gorkom, Miguel Aragón-Calvo, R. van de Weygaert

^*Corresponding author for this work

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

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Abstract

We present the structural and star formation properties of 59 void galaxies as part of the Void Galaxy Survey (VGS). Our aim is to study in detail the physical properties of these void galaxies and study the effect of the void environment on galaxy properties. We use Spitzer 3.6μ and B-band imaging to study the morphology and color of the VGS galaxies. For their star formation properties, we use Hα and GALEX near-UV imaging. We compare our results to a range of galaxies of different morphologies in higher density environments. We find that the VGS galaxies are in general disk dominated and star forming galaxies. Their star formation rates are, however, often less than 1 M⊙ yr-1. There are two early-type galaxies in our sample as well. In re versus MB parameter space, VGS galaxies occupy the same space as dwarf irregulars and spirals.

Original language	English
Title of host publication	The era of multi-Messenger solar physics
Editors	R. van de Weygaert, S. Shandarin, E. Saar , J. Einasto
Publisher	IAU
Pages	600-605
Number of pages	6
DOIs	https://doi.org/10.1017/S1743921316010656
Publication status	Published - 12-Oct-2016

Publication series

Name	Proceedings of the International Astronomical Union
Publisher	IAU
Number	2
Volume	308
ISSN (Print)	1743-9213
ISSN (Electronic)	1743-9221

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The Void Galaxy SurveyFinal publisher's version, 402 KBLicence: Taverne

http://adsabs.harvard.edu/abs/2016IAUS..308..600B

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Beygu, B., Kreckel, K., van der Hulst, T., Peletier, R., Jarrett, T., van de Weygaert, R., van Gorkom, J. H., Aragón-Calvo, M., & van de Weygaert, R. (2016). The Zeldovich Universe: Genesis and Growth of the Cosmic Web . In R. van de Weygaert, S. Shandarin, E. Saar , & J. Einasto (Eds.), The era of multi-Messenger solar physics (pp. 600-605). (Proceedings of the International Astronomical Union; Vol. 308, No. 2). IAU. https://doi.org/10.1017/S1743921316010656

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title = "The Zeldovich Universe: Genesis and Growth of the Cosmic Web ",

abstract = "We present the structural and star formation properties of 59 void galaxies as part of the Void Galaxy Survey (VGS). Our aim is to study in detail the physical properties of these void galaxies and study the effect of the void environment on galaxy properties. We use Spitzer 3.6μ and B-band imaging to study the morphology and color of the VGS galaxies. For their star formation properties, we use Hα and GALEX near-UV imaging. We compare our results to a range of galaxies of different morphologies in higher density environments. We find that the VGS galaxies are in general disk dominated and star forming galaxies. Their star formation rates are, however, often less than 1 M⊙ yr-1. There are two early-type galaxies in our sample as well. In re versus MB parameter space, VGS galaxies occupy the same space as dwarf irregulars and spirals.",

author = "Burcu Beygu and Kathryn Kreckel and {van der Hulst}, Thijs and Reynier Peletier and Tom Jarrett and {van de Weygaert}, R. and {van Gorkom}, {Jacqueline H.} and Miguel Arag{\'o}n-Calvo and {van de Weygaert}, R.",

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year = "2016",

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doi = "10.1017/S1743921316010656",

language = "English",

series = "Proceedings of the International Astronomical Union",

publisher = "IAU",

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Beygu, B, Kreckel, K, van der Hulst, T , Peletier, R, Jarrett, T, van de Weygaert, R, van Gorkom, JH, Aragón-Calvo, M & van de Weygaert, R 2016, The Zeldovich Universe: Genesis and Growth of the Cosmic Web . in R van de Weygaert, S Shandarin, E Saar & J Einasto (eds), The era of multi-Messenger solar physics. Proceedings of the International Astronomical Union, no. 2, vol. 308, IAU, pp. 600-605. https://doi.org/10.1017/S1743921316010656

The Zeldovich Universe: Genesis and Growth of the Cosmic Web . / Beygu, Burcu; Kreckel, Kathryn; van der Hulst, Thijs et al.
The era of multi-Messenger solar physics. ed. / R. van de Weygaert; S. Shandarin; E. Saar ; J. Einasto. IAU, 2016. p. 600-605 (Proceedings of the International Astronomical Union; Vol. 308, No. 2).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

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T1 - The Zeldovich Universe

T2 - Genesis and Growth of the Cosmic Web

AU - Beygu, Burcu

AU - Kreckel, Kathryn

AU - van der Hulst, Thijs

AU - Peletier, Reynier

AU - Jarrett, Tom

AU - van de Weygaert, R.

AU - van Gorkom, Jacqueline H.

AU - Aragón-Calvo, Miguel

AU - van de Weygaert, R.

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Y1 - 2016/10/12

N2 - We present the structural and star formation properties of 59 void galaxies as part of the Void Galaxy Survey (VGS). Our aim is to study in detail the physical properties of these void galaxies and study the effect of the void environment on galaxy properties. We use Spitzer 3.6μ and B-band imaging to study the morphology and color of the VGS galaxies. For their star formation properties, we use Hα and GALEX near-UV imaging. We compare our results to a range of galaxies of different morphologies in higher density environments. We find that the VGS galaxies are in general disk dominated and star forming galaxies. Their star formation rates are, however, often less than 1 M⊙ yr-1. There are two early-type galaxies in our sample as well. In re versus MB parameter space, VGS galaxies occupy the same space as dwarf irregulars and spirals.

AB - We present the structural and star formation properties of 59 void galaxies as part of the Void Galaxy Survey (VGS). Our aim is to study in detail the physical properties of these void galaxies and study the effect of the void environment on galaxy properties. We use Spitzer 3.6μ and B-band imaging to study the morphology and color of the VGS galaxies. For their star formation properties, we use Hα and GALEX near-UV imaging. We compare our results to a range of galaxies of different morphologies in higher density environments. We find that the VGS galaxies are in general disk dominated and star forming galaxies. Their star formation rates are, however, often less than 1 M⊙ yr-1. There are two early-type galaxies in our sample as well. In re versus MB parameter space, VGS galaxies occupy the same space as dwarf irregulars and spirals.

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DO - 10.1017/S1743921316010656

M3 - Conference contribution

T3 - Proceedings of the International Astronomical Union

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EP - 605

BT - The era of multi-Messenger solar physics

A2 - van de Weygaert, R.

A2 - Shandarin, S.

A2 - Saar , E.

A2 - Einasto, J.

PB - IAU

ER -

The Zeldovich Universe: Genesis and Growth of the Cosmic Web

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