ISO-SWS Observations of Stars with Unusual IRAS LRS Characteristics

被引:0
|
作者
S. Deguchi
Y. Yamamura
M. Mizutani
机构
[1] Nobeyama Radio Observatory Minamimaki,Institute of Astronomy Department of Astronomy
[2] SRON,undefined
[3] University of Tokyo,undefined
[4] Bunkyo,undefined
关键词
Silicate; Intensity Ratio; Emission Feature; Unusual Feature; Broad Feature;
D O I
10.1023/A:1001564530042
中图分类号
学科分类号
摘要
Observations of 5 stellar sources with unusual characteristics of IRAS Low Resolution Spectra were made with the SWS on ISO. Observed stars are 4 late-type stars with silicate bands and one planetary nebula. Their IRAS LRS contain somewhat unusual features in respect of the 10/18 µm intensity ratio or narrow emission feature from unknown molecular bands. Some narrow unusual features are confirmed by ISO SWS01 spectra but the broad features were turned out to be false.
引用
收藏
页码:377 / 378
页数:1
相关论文
共 50 条
  • [41] H2 observations of the OMC-1 outflow with the ISO-SWS
    Rosenthal, D
    Bertoldi, F
    Drapatz, S
    MOLECULAR HYDROGEN IN SPACE, 2000, : 231 - 234
  • [42] The relative spectral response calibration of the ISO-SWS
    Vandenbussche, B
    Morris, PW
    Valentijn, EA
    Beintema, DA
    Boxhoorn, DR
    Decin, L
    de Graauw, T
    Feuchtgruber, H
    Heras, AM
    Lahuis, F
    Lorente, R
    Lutz, D
    Roelfsema, PR
    Salama, A
    Shipman, RF
    Van Malderen, R
    Wieprecht, E
    PROCEEDINGS OF THE CONFERENCE ON THE CALIBRATION LEGACY OF THE ISO MISSION, 2003, 481 : 455 - 458
  • [43] Physics and chemistry of planetary nebulae with ISO-SWS
    Salas, JB
    Hony, S
    Pottasch, SR
    Wesselius, PR
    Beintema, DA
    IONIZED GASEOUS NEBULAE: A CONFERENCE TO CELEBRATE THE 60TH BIRTHDAY OF SILVIA TORRES-PEIMBERT AND MANUEL PEIMBERT, 2002, 12 : 160 - 160
  • [44] ISO-SWS observations of the time variability of oxygen-rich mira variables
    Onaka, T
    Yamamura, I
    De Jong, T
    Yamamura, I
    De Jong, T
    Tanabe, T
    Hashimoto, O
    Izumiura, H
    ASTROPHYSICS AND SPACE SCIENCE, 1998, 255 (1-2) : 331 - 338
  • [45] The ISO-SWS spectra of luminous blue variables
    Lamers, HJGLM
    Morris, PW
    Voors, RHM
    vanGent, JI
    Waters, LBFM
    deGraauw, T
    Kudritzki, RP
    Najarro, F
    Salama, A
    Heras, AM
    ASTRONOMY & ASTROPHYSICS, 1996, 315 (02) : L225 - L228
  • [46] ISO-SWS observations of Herbig Ae/Be stars:: HI recombination lines in MWC1080 and CoD -42° 11721
    Benedettini, M
    Nisini, B
    Giannini, T
    Lorenzetti, D
    Tommasi, E
    Saraceno, P
    Smith, HA
    ASTRONOMY & ASTROPHYSICS, 1998, 339 (01): : 159 - 164
  • [47] Quantitative analysis of WC stars:: constraints on neon abundances from ISO-SWS spectroscopy
    Dessart, L
    Crowther, PA
    Hillier, DJ
    Willis, AJ
    Morris, PW
    van der Hucht, KA
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2000, 315 (02) : 407 - 422
  • [48] Calibration issues with data from the ISO-SWS
    Sloan, GC
    Kraemer, KE
    Price, SD
    PROCEEDINGS OF THE CONFERENCE ON THE CALIBRATION LEGACY OF THE ISO MISSION, 2003, 481 : 447 - 449
  • [49] ISO-SWS spectra of [WR] planetary nebulae
    Szczerba, R
    Volk, K
    Górny, SK
    PLANETARY NEBULAE: THEIR EVOLUTION AND ROLE IN THE UNIVERSE, 2003, (209): : 301 - 302
  • [50] ISO-SWS spectra of galaxies: Continuum and features
    Sturm, E
    Lutz, D
    Tran, D
    Feuchtgruber, H
    Genzel, R
    Kunze, D
    Moorwood, AFM
    Thornley, MD
    ASTRONOMY & ASTROPHYSICS, 2000, 358 (02) : 481 - 493