EXPORT: Near-IR observations of Vega-type and pre-main sequence stars

C Eiroa; F Garzón; A Alberdi; D de Winter; R Ferlet; CA Grady; Andrew Collier Cameron; JK Davies; HJ Deeg; AW Harris; Keith Douglas Horne; B Merìn; LF Miranda; B Montesinos; A Mora

EXPORT: Near-IR observations of Vega-type and pre-main sequence stars

C Eiroa, F Garzón, A Alberdi, D de Winter, R Ferlet, CA Grady, Andrew Collier Cameron, JK Davies, HJ Deeg, AW Harris, Keith Douglas Horne, B Merìn, LF Miranda, B Montesinos, A Mora

School of Physics and Astronomy

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

Abstract

We present near-IR JHK photometric data of a sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observing runs ill the period May 1998 to January 1999 and form part of a coordinated effort with simultaneous optical spectroscopy and photo-polarimetry. The near-IR colors of the MS stars correspond in most cases to photospheric colors, although noticeable reddening is present towards a fen objects, and these stars show no brightness variability within the observational errors. On the other hand, the PMS stars show near-IR excesses and variability consistent with previous data.

Original language	English
Pages (from-to)	110-114
Number of pages	5
Journal	Astronomy & Astrophysics
Volume	365
Publication status	Published - Jan 2001

Keywords

stars : emission-line, Be
stars : pre-main sequence
stars : variable : general
infrared : stars
YOUNG STELLAR OBJECTS
HERBIG AE/BE STARS
BETA-PICTORIS
CIRCUMSTELLAR DISK
SYSTEM
SEARCH
DUST
AGE

Cite this

@article{a302049a54d9418c9dd968a2f878f333,

title = "EXPORT: Near-IR observations of Vega-type and pre-main sequence stars",

abstract = "We present near-IR JHK photometric data of a sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observing runs ill the period May 1998 to January 1999 and form part of a coordinated effort with simultaneous optical spectroscopy and photo-polarimetry. The near-IR colors of the MS stars correspond in most cases to photospheric colors, although noticeable reddening is present towards a fen objects, and these stars show no brightness variability within the observational errors. On the other hand, the PMS stars show near-IR excesses and variability consistent with previous data.",

keywords = "stars : emission-line, Be, stars : pre-main sequence, stars : variable : general, infrared : stars, YOUNG STELLAR OBJECTS, HERBIG AE/BE STARS, BETA-PICTORIS, CIRCUMSTELLAR DISK, SYSTEM, SEARCH, DUST, AGE",

author = "C Eiroa and F Garz{\'o}n and A Alberdi and {de Winter}, D and R Ferlet and CA Grady and Cameron, {Andrew Collier} and JK Davies and HJ Deeg and AW Harris and Horne, {Keith Douglas} and B Mer{\`i}n and LF Miranda and B Montesinos and A Mora",

year = "2001",

month = jan,

language = "English",

volume = "365",

pages = "110--114",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "EDP SCIENCES S A",

}

TY - JOUR

T1 - EXPORT: Near-IR observations of Vega-type and pre-main sequence stars

AU - Eiroa, C

AU - Garzón, F

AU - Alberdi, A

AU - de Winter, D

AU - Ferlet, R

AU - Grady, CA

AU - Cameron, Andrew Collier

AU - Davies, JK

AU - Deeg, HJ

AU - Harris, AW

AU - Horne, Keith Douglas

AU - Merìn, B

AU - Miranda, LF

AU - Montesinos, B

AU - Mora, A

PY - 2001/1

Y1 - 2001/1

N2 - We present near-IR JHK photometric data of a sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observing runs ill the period May 1998 to January 1999 and form part of a coordinated effort with simultaneous optical spectroscopy and photo-polarimetry. The near-IR colors of the MS stars correspond in most cases to photospheric colors, although noticeable reddening is present towards a fen objects, and these stars show no brightness variability within the observational errors. On the other hand, the PMS stars show near-IR excesses and variability consistent with previous data.

AB - We present near-IR JHK photometric data of a sample of 58 main-sequence, mainly Vega-type, and pre-main sequence stars. The data were taken during four observing runs ill the period May 1998 to January 1999 and form part of a coordinated effort with simultaneous optical spectroscopy and photo-polarimetry. The near-IR colors of the MS stars correspond in most cases to photospheric colors, although noticeable reddening is present towards a fen objects, and these stars show no brightness variability within the observational errors. On the other hand, the PMS stars show near-IR excesses and variability consistent with previous data.

KW - stars : emission-line, Be

KW - stars : pre-main sequence

KW - stars : variable : general

KW - infrared : stars

KW - YOUNG STELLAR OBJECTS

KW - HERBIG AE/BE STARS

KW - BETA-PICTORIS

KW - CIRCUMSTELLAR DISK

KW - SYSTEM

KW - SEARCH

KW - DUST

KW - AGE

UR - http://www.scopus.com/inward/record.url?scp=0034791507&partnerID=8YFLogxK

M3 - Article

SN - 0004-6361

VL - 365

SP - 110

EP - 114

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

ER -

EXPORT: Near-IR observations of Vega-type and pre-main sequence stars

Abstract

Keywords

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